The galaxy presents a somewhat elongated, cigar-shaped morphology, potentially indicative of an elliptical galaxy or a spiral galaxy viewed at a high inclination. The central region exhibits a bright, concentrated luminosity, appearing nearly spheroidal. Moving outwards, the light distribution becomes more diffuse and elongated, with a clear decrease in surface brightness towards the apparent edges of the galaxy. There is evidence of asymmetry or disturbance in the morphology of the disk, with an apparent bulge or arm on one side. The general color profile seems to redden toward the core, although this may simply be due to seeing conditions, which is potentially suggestive of an older stellar population being dominant in the central regions. The overall appearance suggests that the galaxy is not undergoing a major merging event, although there are minor disturbances that could indicate tidal interactions. 
