The galaxy presents as a smooth, elliptical morphology with a concentrated central bulge. There is a color gradient visible, shifting from a more yellowish-orange core to greenish hues in the outer regions, suggesting a variation in stellar populations or dust content. The galaxy appears relatively undisturbed, showing no prominent signs of tidal features or major mergers. The overall structure indicates a system dominated by an older stellar population, particularly within the central bulge, while the presence of the greenish hues could indicate some ongoing, albeit limited, star formation in the outer regions. The light distribution is centrally concentrated, with a gradual decline in intensity outwards.
