The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. There is no clear evidence of spiral arms or significant disk features. The color profile indicates a population of older stars, particularly in the central region, with a yellowish-orange hue dominating. The outer regions of the galaxy show a slight decrease in surface brightness, with the color becoming subtly bluer, hinting at a younger stellar population at the outskirts, though overall star formation activity appears to be low. There are no obvious signs of ongoing mergers or tidal disturbances that are visible in the image. The overall morphology appears settled and relaxed.
