The galaxy presents as a relatively smooth and elliptical object. Its color suggests an older stellar population. The galaxy appears nearly circular, with an axis ratio very close to 1, indicating it is close to face-on. The light distribution appears centrally concentrated, typical of elliptical galaxies. There's no clear evidence of spiral arm structure or significant dust lanes, supporting its classification as an elliptical galaxy. The galaxy shows a gradual decrease in brightness from its center to its outer regions, without any abrupt edges or distinct features. The galaxy appears isolated, without signs of major disturbances or ongoing mergers.
