The galaxy presents a generally smooth, elliptical morphology. It appears largely featureless, with no obvious spiral arms or bar structures visible. The light distribution is concentrated towards the center, with a gradual decrease in luminosity towards the edges. The galaxy exhibits a yellowish-orange hue, suggesting a population of older stars and a relatively low rate of ongoing star formation. There is no noticeable dust lane or significant presence of blue light indicative of young, hot stars. The galaxy's shape is nearly round, showing no signs of strong tidal disturbances or ongoing mergers, although a very subtle asymmetry cannot be completely ruled out.
