The galaxy appears to be a relatively smooth, elliptical galaxy. It presents with a high degree of central concentration, displaying a bright, well-defined core that diminishes gradually outward. The color profile suggests a relatively evolved stellar population, with a reddish-yellow hue that is consistent with older stars. No distinct features such as spiral arms or dust lanes are discernible. The overall shape is close to round and there is no indication of any major gravitational disturbances or ongoing mergers in this image, suggesting a stable, relaxed system.
