The galaxy presents as an elliptical or lenticular type, displaying a high degree of smoothness with a centrally concentrated, bright bulge. The galaxy exhibits a generally rounded morphology, with minimal discernible disk features or spiral arms. The color profile suggests an older stellar population, with a dominant red-yellow hue in the central bulge and a subtle blue-green tinge in the outer regions, hinting at some ongoing, though limited, star formation activity. There is no obvious evidence of major mergers or significant tidal disturbances in the immediate vicinity, although minor asymmetries could suggest past interaction or accretion events. The overall structure appears relatively undisturbed and evolved.
