The galaxy presents as a relatively smooth, centrally concentrated elliptical type. It exhibits a bright core that gradually diffuses outward, forming a somewhat flattened or "in between" shape, neither perfectly circular nor highly elongated. There is minimal evidence of spiral arms or distinct substructures, and no strong indication of an ongoing major merger event; however, some minor disturbances are a possibility. The overall color appears somewhat redder than average suggesting an older stellar population and comparatively lower levels of ongoing star formation. The apparent size is relatively small, consistent with a galaxy at a significant cosmological distance.
