The galaxy appears as a centrally concentrated object, exhibiting a smooth, largely featureless morphology. Its overall shape is elliptical, presenting as moderately rounded with an observed axis ratio close to unity. There is a clear color gradient visible within the galaxy, trending from yellow at the core to red as you move toward the outer edges. This suggests a stellar population that is redder and therefore most likely older in the inner regions. No spiral arm structure or significant dust lanes are discernible, which implies that this is not an actively star-forming galaxy. The galaxy lacks any signs of active galactic nuclei or recent major mergers. Minor disturbances cannot be ruled out based on the image alone.
