The galaxy appears as a single, centrally concentrated object. The light profile seems relatively smooth and undisturbed. The color of the galaxy is somewhat reddish, indicating that it may be composed of older stars, or that there is dust obscuring shorter wavelengths. There is not much indication of spiral arms or other distinct features. It could be an elliptical galaxy. The lack of distinct morphological features suggest that the galaxy is unlikely to be undergoing a major merger, although it may be experiencing minor interactions. The galaxy's overall structure suggests it may be evolving passively.
