The galaxy presents as a somewhat diffuse, elliptical-shaped structure. The central region exhibits a concentrated luminosity, suggesting a substantial stellar population and potentially a supermassive black hole at the core. There is a gradual decrease in luminosity from the core to the outer edges, giving it a smooth appearance overall. Faint hints of bluer colors are visible in the galaxy's outer regions, possibly indicating areas of recent star formation. No strong spiral arm structures or other features indicative of a disk galaxy are apparent. There is no indication of a significant ongoing merger or interaction with another galaxy, the galaxy appears relatively undisturbed.
