The galaxy presents a smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, appearing nearly round. The core region shows a yellowish hue, suggestive of an older stellar population. There is a faint, diffuse halo surrounding the central region. The galaxy lacks any discernible spiral arm structures or dust lanes. There are no signs of any major mergers or tidal disturbances, indicating a relatively undisturbed system. The galaxy appears to be a mature system with little active star formation.
