The galaxy presents a smooth, elliptical morphology with a bright, concentrated central bulge. It exhibits a general lack of distinct spiral arm structures, suggesting it may be classified as an early-type galaxy. The light profile appears relatively uniform, with a gradual decrease in intensity from the core outwards. There is a slight elongation and a hint of asymmetry present in the outer regions, potentially indicating minor gravitational interactions or past merger events. A smaller, fainter object is visible in close proximity, possibly a companion galaxy or a tidal feature resulting from interaction. The overall color appears relatively red, implying a population of older stars and a lower rate of current star formation.
