The galaxy presents an overall elliptical morphology. Its light profile appears smooth and centrally concentrated, indicative of an early-type galaxy. The central region is brighter and whiter than the outer regions. There is a minor disturbance evident. The blue tint in the center suggests a younger stellar population or recent star formation, although the galaxy seems to be primarily dominated by older stars that impart a somewhat redder hue. The outer edges of the galaxy appear to fade gradually into the background sky, consistent with a low surface brightness halo. There is only a single nucleus.
