The galaxy presents as a relatively smooth, elliptical-like structure with a diffuse halo. Its core appears brighter than its outer regions, suggesting a concentration of older stellar populations towards the center. The overall color is generally consistent, with a slight tendency towards redder hues. No prominent spiral arms or dust lanes are readily discernible. The morphology is indicative of a galaxy that has undergone significant evolution, possibly through mergers, leading to a homogenized stellar distribution. There is no obvious tidal debris or close companions suggesting recent major merger events. Marginal irregularities are visible on the outskirts, which could suggest some past minor interactions. 