The galaxy presents as a centrally concentrated, smooth, elliptical object. It exhibits a yellow-orange hue, suggesting a population dominated by older stars. The overall shape is somewhat elongated, but not dramatically so. There is no visible evidence of spiral arms or significant dust lanes. The lack of distinct features suggests the galaxy is not currently undergoing major star formation. There is no evidence of any ongoing major merger events, though a minor disturbance cannot be completely ruled out. The galaxy appears to be relatively isolated.
