The galaxy appears to be elliptical in shape, with a smooth, relatively featureless morphology. It presents a concentrated central bulge with a gradual decrease in luminosity towards the outer regions. No distinct spiral arms or prominent dust lanes are discernible. The color indices suggest a population of older stars, indicative of a passively evolving system with low current star formation rate. Based on its apparent size and estimated distance derived from photometric redshift, the galaxy is likely a massive object, potentially of the order of 10^10 to 10^11 solar masses. No signs of ongoing major mergers or significant tidal disturbances are visible. The overall visual impression is that of a quiescent elliptical galaxy.
