The galaxy presents as a relatively smooth, elliptical structure. It is centrally concentrated, displaying a bright core region, but appears largely featureless. The isophotes are generally round. There appears to be no significant tidal distortion or indication of a major merger event in recent history. There appears to be a minor disturbance nearby, with a faint tail extending outward. Its color index suggests a population dominated by older stars. There is little evidence of ongoing active star formation. The galaxy's overall appearance is consistent with a spheroidal system, likely a massive galaxy at a considerable distance.
