The galaxy presents as a single, dominant, elliptical-like object with a smooth, concentrated central bulge. It exhibits a yellowish-orange hue, suggesting a population dominated by older stars. No distinct spiral arms or significant dust lanes are apparent. The galaxy appears relatively undisturbed, without major signs of tidal interactions or recent mergers. Its round shape is close to spherical, which fits well with the hypothesis that it is an elliptical galaxy. The galaxy is rather bright. Star formation appears to be low within the galaxy. Overall, the galaxy displays characteristics consistent with an evolved, massive system with minimal ongoing star formation.
