The galaxy presents as a relatively smooth, elliptical-shaped object. Its color is predominantly a soft, bluish-white. There is a bright, concentrated central bulge that fades into a diffuse halo. The lack of strong spiral arm structures or dust lanes suggest the galaxy is likely an early-type galaxy. The slight elongation implies that it is not perfectly spherical, but rather somewhat flattened. There is no obvious evidence of ongoing mergers or major disturbances in its structure, although there is a hint of minor irregularity in the outer regions. The colors suggest older stellar populations within, with a possible low level of ongoing or recent star formation. Overall, it is likely a relatively quiescent galaxy with a substantial mass and correspondingly low star formation rate.
