This galaxy presents as an elliptical or lenticular type. The light distribution is centrally concentrated with a smooth, diffuse halo extending outward. The core exhibits a bright, yellowish-white hue. A bluer, less intense region surrounds the central bulge, transitioning smoothly into the outer halo. There is no visible spiral arm structure or dust lane obscuration. Overall, the galaxy appears relatively undisturbed, without evidence of major mergers or tidal interactions. The morphology suggests a system dominated by an older stellar population with relatively low levels of ongoing star formation.
