The galaxy appears to be a relatively smooth, elliptical-type galaxy. The core exhibits a high degree of central concentration with a bright, yellowish-white hue. Moving outward from the core, the light gradually diminishes. The galaxy's overall shape is nearly circular with a moderate amount of fuzziness and a smooth gradient in its luminosity profile. There is no obvious indication of spiral arm structure or significant dust lanes, suggesting a lack of recent major star formation. Minor disturbances in the form of low-level asymmetrical features are subtle but present, potentially hinting at past or ongoing minor interactions with smaller galaxies. The outer regions are barely discernible, appearing as a faint halo surrounding the brighter central part of the galaxy.
