The galaxy presents as a single, relatively smooth, and concentrated luminous object. The overall shape appears approximately round, exhibiting a slight deviation from perfect circularity. There is a color gradient observed from the center outward, with the core region appearing more yellow-white, transitioning to a more reddish hue in the outer regions. The luminosity distribution indicates a centrally concentrated profile, typical of an elliptical galaxy. There is no significant evidence of spiral arms or a distinct disk structure. The galaxy appears relatively undisturbed, with only minor asymmetries or tidal features visible, suggesting the absence of any major recent merging activity. Overall, the galaxy seems to be quite massive and has low levels of recent star formation.
