The galaxy presents as a relatively smooth, elliptical object. It exhibits a centrally concentrated luminosity profile, with a bright core that gradually fades into the surrounding halo. The overall shape is close to circular. There is a subtle color gradient, suggesting a slightly bluer outer region compared to the central core. No distinct spiral arm structures or prominent dust lanes are visible. There are no signs of any ongoing major merger events, though there may be minor disturbances present. The galaxy is likely a relatively massive system with a low star-formation rate.
