The galaxy appears to be an elliptical galaxy. It presents a smooth, relatively featureless morphology with a concentrated central bulge. The light distribution seems symmetric and concentrated with a radial gradient and without spiral arm structures. The color index suggests a population of older stars, likely consisting of Population II stars. The overall luminosity implies a substantial stellar mass. Based on its morphology it is likely a quiescent galaxy, with little to no ongoing star formation. No interactions or merging events are obviously visible.
