The galaxy presents a generally smooth, elliptical morphology. It exhibits a bright, concentrated central bulge that diminishes in luminosity towards the outer regions. There is a suggestion of a flattened disk-like structure surrounding the bulge, but it is not clearly defined. The color profile indicates a population of older stars, as evidenced by the reddish-yellow hue, potentially signifying a lower rate of ongoing star formation. It appears relatively undisturbed, without major signs of tidal interactions or mergers. Overall, this galaxy likely represents a mature system with a significant mass, possibly undergoing a period of quiescence in star formation activity.
