The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The primary color appears to be a bluish-white, indicating the presence of a population of younger, hotter stars, with a redshift measurement that places it at a significant cosmological distance. There appears to be some reddish components, but no discernable spiral arms or other defined structures beyond the overall smooth distribution of light. It exhibits a shape that appears to be somewhere in between round and elongated. No signs of major mergers are apparent, although there is a faint suggestion of minor disturbance. Overall, it seems like an isolated, relatively undisturbed system.
