The galaxy appears as a centrally concentrated, elliptical-like system. The light is relatively smooth, with a diffuse profile extending outwards from a bright central core. There is a color gradient, trending from a whiter central region to a slightly redder periphery. No distinct spiral arm structures or dust lanes are visible. The overall shape is somewhat irregular, not perfectly spherical, hinting at possible minor interactions or internal dynamic processes. Based on the red color, the stellar population is likely dominated by older stars with a relatively low ongoing star formation rate. The system is likely a galaxy in the low to mid-range mass. There is no evidence of a major ongoing merger, although some minor disturbance cannot be ruled out.
