The galaxy appears to be an elliptical galaxy, exhibiting a smooth, relatively featureless morphology. The light profile suggests a centrally concentrated bulge with a gradual decrease in luminosity towards the outer regions. The galaxy has a moderate elongation, appearing more cigar-shaped than perfectly circular. There is no clear evidence of spiral arms or a distinct disk component. The galaxy's color suggests an older stellar population, with a redder hue in the core gradually transitioning to slightly bluer tones in the periphery. There is no visible dust lane, and no signs of major mergers or tidal disturbances are apparent. The overall appearance is consistent with a well-evolved, passively evolving galaxy.
