The object presents as a generally smooth, centrally concentrated galaxy. Its morphology appears elliptical, or potentially a lenticular galaxy viewed close to face-on, lacking prominent spiral arm structures. The central bulge exhibits a high degree of luminosity, suggestive of a significant population of older stars. The light profile fades gradually from the core, with no sharp truncations or distinct features. The galaxy appears relatively isolated, with no immediately apparent signs of major interaction or tidal disturbances. There is minimal, if any, indication of ongoing, intense star formation in the visible bands based on the color and morphology. Overall the galaxy presents as a well-defined, relatively undisturbed system.
