The galaxy presents as a single, centrally concentrated luminous region, suggesting a classification as elliptical or potentially lenticular. The galaxy exhibits a smooth, symmetric morphology with a largely featureless appearance, indicating minimal dust lanes or spiral arm structures within the limits of resolution. The light distribution appears relatively even, becoming more diffuse towards the outer edges. A slight color gradient is observed, with the central region appearing more yellow-white, possibly indicating an older stellar population. The outer regions show a faint reddish color cast, but further analysis would be required to determine the nature of this extended light. There is no indication of any recent or ongoing major merger activity or tidal disturbances in this single frame. 
