The galaxy appears as a relatively smooth, elliptical object. It is elongated, but not highly so, possessing an intermediate shape between round and cigar-shaped. The light distribution is centrally concentrated, fading gradually outwards. No distinct spiral arms or bar structures are visible. There is a very slight hint of a disk. There are no signs of major mergers or significant tidal disturbances, although very minor disturbances could be present. The galaxy exhibits a redder color profile, suggesting a population of older stars and a relatively low rate of star formation. It appears as a galaxy that has mostly completed its evolution.
