The galaxy presents a largely smooth, centrally concentrated light distribution. It appears elliptical in shape, deviating slightly from perfect circularity. The core exhibits a bright, concentrated luminosity, suggesting a significant population of older stars and potentially a supermassive black hole at the galactic center. A faint, diffuse halo surrounds the brighter central region, indicating a gradual decrease in stellar density with increasing distance from the center. There's a subtle color gradient, transitioning from a slightly bluer hue in the outer regions to a more yellowish-red color toward the core, indicative of varying stellar populations and ages. No distinct spiral arm structures or prominent dust lanes are visible. There is no sign of a major ongoing merger. Faint asymmetries are possibly present in the outer reaches of the galaxy. Overall, the galaxy appears to be a relatively massive, evolved system.
