The galaxy appears to be a luminous elliptical, exhibiting a smooth, centrally concentrated light profile. Its shape is close to circular. There is no obvious indication of spiral arm structure or a prominent disk. The core region is significantly brighter and more yellow, possibly indicating an older stellar population. The outskirts are dimmer and bluer, suggesting some ongoing star formation, however, it appears to be low. There is no visible sign of a major merger or significant tidal disturbance in the galaxy's structure.
