The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge with a diffuse halo extending outwards. The color gradient suggests an older stellar population, with a yellowish-red hue dominating the central region, possibly indicating a lack of significant ongoing star formation. There's little evidence of spiral arms or significant dust lanes. The overall shape is somewhat elongated, but without any obvious signs of a major merger or tidal disruption, though a minor disturbance cannot be ruled out. Based on its apparent size and morphology, the galaxy seems to be a mature system.
