The galaxy presents a generally smooth morphology, with an elliptical-like shape predominating. There is likely an absence of prominent spiral arms or other distinct features. The galaxy appears to be undergoing little to no significant star formation activity, and is a relatively large galaxy. We see some disturbances around the object, and the source may be undergoing a minor merger. The color profile suggests a population of older stars, typical of elliptical galaxies, with an overall redder hue.
