The galaxy presents as an elliptical or lenticular type, with a smooth, concentrated light profile. Its core region exhibits a bright, golden hue, suggesting a significant population of older stars. The light appears to fade gradually outward from the center, implying a lack of distinct spiral arms or significant dust lanes. There are only minor disturbances. The overall shape is tending towards in between roundedness and in between ellipticity. The object displays a minor level of interaction or merger activity.
