The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated luminosity profile, with a bright core that gradually fades outward. The galaxy's overall shape is somewhat elongated. There's a lack of any discernible spiral arm structure or prominent dust lanes. The color is consistent with an older stellar population, presenting as a relatively red color, with a relatively low star formation rate. No signs of major mergers or significant disturbances are visible. The galaxy is moderately luminous. 
