The galaxy presents as a somewhat elliptical, though mostly round, structure. The core region exhibits a brighter, more concentrated luminosity, suggesting a higher density of stars and possibly a central supermassive black hole actively accreting material. The outer regions of the galaxy show a gradual decrease in luminosity, with a smooth transition outwards. There is a hint of a disclike structure. The overall color appears yellowish-white, with a possible blueish tint. The galaxy does not show any obvious signs of major disturbances or ongoing mergers.
