The galaxy presents as a largely smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing mostly round, though possibly slightly elongated along a non-distinguishable axis. The central region displays a bright, prominent core. A diffuse halo or envelope extends outwards from the core, with a gradual decrease in luminosity, suggesting a significant stellar population within the spheroid. Faint color variations are seen, with the core appearing more yellow/orange. The disk structure appears to be mostly quiescent. A lack of significant dust lanes or prominent spiral arm features suggests a relatively low star formation rate. There may be some minor disturbances in the outer regions, but no major mergers or interactions are readily apparent.
