The galaxy appears to be relatively small, with an estimated size of approximately 6 arcseconds across. It exhibits a somewhat disturbed morphology, possibly indicative of a minor merger event or gravitational interaction. While a significant portion of it is relatively smooth, there are areas of patchiness and asymmetry. The core is difficult to resolve in great detail, but appears somewhat bright. The overall color profile suggests a population of older stars, with slightly diminished ongoing star formation. There appears to be no major disturbance or strong tidal features.
