The galaxy presents as a fairly smooth, elliptical morphology. It displays a concentrated central bulge, with a gradual decrease in luminosity towards its outer edges. No distinct spiral arm structures or features indicative of ongoing major mergers are apparent. There are no large tidal tails or distortions, although there appears to be some minor disturbance in the morphology. The galaxy exhibits a predominantly round shape. The color profile suggests a population of older stars, although there also appears to be a small amount of active star formation, or a population of young stars.
