The galaxy presents a complex morphology. There is a dominant central region, intensely bright and appearing slightly blue-shifted, possibly indicating active star formation. Extending outwards from the central region are diffuse, less luminous structures appearing reddish. These structures are likely stellar populations of older stars. 

The overall shape suggests a disk-like structure, potentially with spiral arms that are not well defined, or perhaps a galaxy with a prominent bulge and a disrupted or irregular disk. There's a hint of asymmetry, with one side appearing slightly more extended or distorted than the other.

There may be a faint tidal tail or bridge of material extending from the main body. This might be indicative of past interaction with another galaxy, although no clear companion is immediately apparent within the immediate vicinity in this image. The system appears to be relatively isolated within the field of view.
