The galaxy presents as a moderately luminous object with a smooth, elliptical morphology. The color gradient suggests a population of older stars, with a central concentration of light and a more diffuse, extended halo. There is a noticeable lack of discernible spiral arms or dust lanes. The overall appearance indicates a relatively quiescent galaxy, potentially an early-type galaxy nearing the red sequence. It appears relatively undisturbed, showing no strong signs of recent major merger activity, though there is a subtle asymmetry. The core is bright and centrally condensed. The outer edges of the halo appear to fade smoothly into the background, suggesting a gradual decrease in stellar density with increasing radius.
