The galaxy presents as a centrally concentrated, elliptical morphology. It exhibits a smooth light distribution, lacking any prominent spiral arms or distinct features typically associated with disk galaxies. The color profile is generally consistent across the galaxy, displaying a yellowish-orange hue. This suggests an older stellar population is dominant, with minimal ongoing star formation. The galaxy appears relatively isolated, without obvious signs of tidal interactions or major disturbances, although subtle asymmetries may indicate minor gravitational influences. The overall appearance is consistent with a massive elliptical galaxy, likely with a significant contribution from evolved stars. The size and shape are indicative of a well-formed, early-type galaxy residing at a considerable distance.
