The galaxy exhibits a largely elliptical morphology, appearing mostly smooth in texture with a high degree of central concentration. Its color is largely indicative of a relatively evolved stellar population with a redder hue. There is a very low degree of identifiable substructure or disk features, nor significant signs of recent or ongoing mergers or major disturbances. The galaxy displays no obvious spiral arm structure or active star-forming regions. The rounded shape is neither perfectly circular nor particularly elongated. There appears to be some possible minor disturbance present.