The galaxy appears as a singular, concentrated object, exhibiting a generally elliptical morphology. The light profile suggests a centrally concentrated distribution, fading gradually outwards. Its color is predominantly yellow to orange, indicating an older stellar population with minimal ongoing star formation. There are no prominent spiral arm structures or dust lanes visible within the galaxy. The overall impression is that of a relatively smooth, evolved galaxy likely composed of older stars. It has a high degree of symmetry and no obvious tidal features.
