The galaxy presents as an elliptical morphology with a moderate degree of ellipticity. It exhibits a smooth, centralized concentration of light, indicative of an older stellar population. The core displays a brighter, yellowish hue, possibly indicating a higher density of older stars and a diminished presence of recent star formation. Fainter, bluer hues surround the central bulge, suggesting regions with more recent star formation. The overall light distribution follows a concentrated profile, with the majority of light contained within a relatively small radius. No spiral arms or distinct disk features are readily apparent. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions.
