The galaxy presents a complex morphological structure. It exhibits characteristics consistent with a possible ongoing galactic merger or interaction. There appears to be a brighter, more spherical component likely representing the core of one galaxy, and a more diffuse, disk-like component that may be either a second interacting galaxy or a tidally disrupted structure. 

The color gradient suggests a redder central region, which could indicate an older stellar population or significant dust extinction. The outer regions are comparatively bluer, potentially indicating ongoing star formation. The disk appears elongated with signs of distortion in its morphology, possibly due to gravitational interactions. The galaxy as a whole appears somewhat smooth in overall structure, but with some irregularities that are probably indicative of disturbed morphology.