The galaxy presents as a centrally concentrated, smooth, and luminous object. It appears to be largely featureless, with a distinct lack of spiral arms or prominent dust lanes. The light profile suggests a spheroidal shape, nearly circular. The color gradient indicates a population of older stars. It is primarily a yellow-orange hue, suggesting an aging stellar population with minimal recent star formation. There is a very slight disk surrounding the center. There is no indication of strong tidal interactions or recent merger events.
