The galaxy presents as a centrally concentrated object with a relatively smooth morphology. The primary body exhibits a dominant, bright central bulge. The surrounding light is distributed in an elliptical pattern. There is little indication of spiral arm structure or significant disk features. The galaxy appears slightly elongated but is generally round. Overall, there is no obvious evidence of a recent major merger event. It may be a lenticular galaxy, dominated by an older stellar population with reduced star formation.
