The main imager is the Near Infrared Camera. It has ten 2048x2048 sensors. They're configured in two kinda-independent groups with separate optics. Each group uses one of those sensors for longer wavelengths (so you get two lots of 2048x2048), and four of them for shorter wavelengths (so you get two lots of 4096x4096). The two modules can (and I guess usually will) be pointed at adjacent regions of the sky; I expect they'll overlap them a bit so you'll get slightly under 4096x2048 for the long wavelengths and slightly under 8192x4096 for the short. These are monochrome sensors but they have an array of filters they can swap in to measure different wavelengths.
There are several other instruments, including some other imagers.