They can use this as a blue print for how to assemble spaceships in orbit.
Indeed, if completed this will be an extraordinary example of space construction.
Having done some amateur astronomy with a small Newtonian telescope let me explain why it's hard: that big mirror is not spherical but rather a section of a parabola. The parabolic shape allows incoming light (which are travelling parallel since it comes from distance measured in light years) to be focused to the detector at the focal point. Using a spherical mirror instead of a parabolic mirror will cause a major optical defect in focusing called "spherical aberration" which will make this telescope useless.
Because the primary mirror is a section of a parabola it means all the mirror segments are actually different and not interchangeable. Not only that when you assemble a segmented primary mirror each segment have to be aligned accurately to a small fraction of the the wavelength of the light you're measure (in other words, the mirror has to look "smooth" on the scale of visible light photons), so for visible light we're talking accuracy of around 10 nanometers. If a segmented mirror is not correctly aligned it's as if a single big glass mirror has lots of bumps in it which will not be acceptable.
For that sort of accuracy it means both the overall mirror segments have to be aligned to quite good accuracy, then each mirror segment have to be further finely aligned using machinery built into the back of them called "active optics" which basically means lining up the back of the mirror with lots of tiny actuators that can adjust them.
JWST for example uses this technology and has seven actuators per mirror segments (one per corner and one in the middle, with 18 segments all together). This big Chinese telescope will need at least 7 per segment as well. Note that these nanometer accurate actuators can only move very tiny distances, so the overall mirror assembly still has to be done to very high degree of accuracy first.
You might hear the world "adoptive optics" when dealing with reflecting telescopes. This is a similar technology but involves much more actuators per mirror segments. These actuators are not only responsible for tilting the segments to align them, but also flexing the mirror by tiny amount (and adjusting the flex in real time) to compensate for atmosphere seeing. Since space telescopes are above the atmosphere they do not require this much more elaborate system.