The galaxy presents a largely smooth morphology, appearing generally elliptical. The primary body exhibits a concentrated central bulge, with a gradual decrease in luminosity towards its outer regions. The light distribution suggests a relatively evolved stellar population, with a dominant reddish hue. There is a suggestion of some dust attenuation or differential reddening within the galaxy, as indicated by the color variations across its extent. There is a very small possible disk, and it does not appear to show signs of active star formation within the optical bands, though its redshift indicates it is significantly distant. There is a very nearby object, and that could represent a slight disturbance. The light suggests it is not undergoing a major merger. The primary axis seems slightly elongated, but it is generally round.
