The galaxy appears to be a relatively compact object with a bright, nearly unresolved core. There is a noticeable color gradient from the core outward, shifting from a bluer, possibly younger stellar population in the central region to a redder, potentially older population in the surrounding halo or disk. 

There is some subtle indication of asymmetry in the outer regions, which may suggest a minor disturbance or interaction. The image resolution limits a definitive classification; however, the overall morphology appears closer to a smooth elliptical galaxy or perhaps a lenticular galaxy with a significant bulge. A faint extension can be seen on one side, which could be an indication of tidal features caused by minor interactions.
