The galaxy presents as a centrally concentrated, elliptical morphology. It exhibits a smooth light distribution, lacking prominent spiral arm structures or distinct dust lanes. The overall color appears yellowish-white, suggesting a population of older stars. The round appearance suggests that it is an elliptical galaxy. There are no other galaxies nearby that may indicate that it may be a merging system. It appears to be isolated. There is no strong evidence of ongoing star formation. It is a massive galaxy that it relatively inactive.
