This galaxy appears to be a relatively smooth, elliptical-type galaxy at a considerable distance, as evidenced by its small angular size. Its light profile suggests a concentrated central bulge with a gradual decrease in luminosity outwards. The color appears generally redder, suggestive of an older stellar population dominated by evolved stars, although there are hints of bluer regions within the galaxy. The galaxy seems largely undisturbed, showing no obvious signs of a recent major merger or significant tidal interaction. The overall shape is neither perfectly spherical nor highly elongated. There is no discernible spiral arm structure or prominent dust lane visible. The galaxy's morphological features are consistent with a galaxy that has largely exhausted its gas supply for star formation.
