The galaxy presents as an elliptical morphology, exhibiting a smooth, largely featureless structure. The core displays a concentrated luminosity gradient, transitioning to a more diffuse halo. Color gradients indicate a higher concentration of older stellar populations in the central region, gradually shifting to a slightly bluer hue in the outer regions. The galaxy appears relatively undisturbed, showing no obvious signs of recent major mergers or significant tidal interactions. There might be minor disturbance present. Based on the overall appearance and redshift, the galaxy represents a massive system, likely composed of a significant fraction of evolved stars.
