The galaxy presents as a centrally concentrated elliptical morphology, exhibiting a smooth, diffuse light distribution with a generally spheroidal shape. There is little evidence of spiral arm structure or significant dust lanes. The core region is bright and appears yellowish-white, potentially indicating an older stellar population dominating the central mass. The outer regions show a gradual decrease in luminosity, fading into the background sky. Subtle color gradients are discernible, with the outer halo potentially exhibiting a slightly bluer hue compared to the core, suggesting the presence of some younger stars or differences in metallicity. No strong tidal features or signs of ongoing major mergers are apparent, though minor disturbances cannot be ruled out based on this image alone. The overall appearance suggests a relatively evolved, massive system, possibly with a suppressed star formation rate.
