The galaxy presents as a smooth, elliptical-like structure with a distinct color gradient. The central region exhibits a bright, reddish-orange hue, suggesting a concentration of older stellar populations and/or dust obscuration. Moving outwards, the color shifts towards a greenish tinge, which could indicate the presence of younger stars or a different dust composition. The overall shape appears somewhat elongated, deviating slightly from a perfect circle. There are no visually discernible spiral arms or prominent features suggesting ongoing major mergers. The galaxy appears relatively undisturbed, showing subtle asymmetries that may point to minor tidal interactions or internal dynamics influencing its morphology. The light distribution suggests a centrally concentrated mass profile, typical of elliptical galaxies. The faintness of the outer regions compared to the core implies a declining stellar density with increasing radial distance.
