The galaxy appears as a roughly circular, centrally concentrated object. It exhibits a smooth, diffuse profile, lacking any prominent spiral arms, bars, or distinct features suggestive of ongoing mergers or major disturbances. A color gradient is present, transitioning from a more yellowish-orange core to a greenish-blueish outer region. This color distribution suggests the presence of older stellar populations in the galactic center, with relatively lower levels of ongoing star formation activity compared to the outer regions. The overall morphology is consistent with that of an elliptical galaxy or a lenticular galaxy seen face-on, and is likely a very massive galaxy. The lack of visible substructure indicates that it is either a well-mixed galaxy or is at too great a distance for finer details to be resolved.
