The galaxy presents as a single, relatively smooth object. Its morphology is primarily elliptical, displaying a high degree of sphericity with minimal discernible features. Coloration is generally yellow-orange, potentially indicating an older stellar population. The luminosity profile suggests a centralized concentration of light, with brightness diminishing gradually outwards. There is no apparent spiral structure, bar, or significant dust lane visible. It appears isolated, showing no obvious signs of recent or ongoing major merger activity, although minor disturbances cannot be ruled out. Based on its redshift, the galaxy is at a considerable distance.
