The galaxy presents a generally smooth, elliptical morphology. It appears largely spheroidal with minimal discernible disk features. There is a high degree of central concentration, with a bright, unresolved core. The color profile suggests a relatively evolved stellar population. The overall color is red, indicating a dominance of older stars. There is a faint suggestion of a very minor asymmetry extending outwards in one direction from the main body. The galaxy appears fairly isolated and unperturbed; there is no significant evidence of ongoing or recent major mergers or tidal interactions.
