The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a slightly elliptical shape, appearing more "in between" round and elongated, with a hint of a disk-like structure but no strong spiral arms. A central bulge region can be seen, slightly brighter in color than the rest of the galaxy. There are no strong indications of any on-going major merger event, though a minor disturbance or subtle feature could be present. The overall color suggests a population of older stars, with little evidence of recent, intense star formation. The galaxy shows an overall redder appearance, with a few bluer regions, possibly indicating some younger stellar populations in localized areas. The observed size appears relatively compact.
