The galaxy presents a somewhat smooth morphology, appearing primarily elliptical in shape. There appears to be ongoing or recent merger activity, as indicated by the slight elongation and the presence of some minor disturbances in its overall structure. The light distribution is concentrated towards the center. There is a general lack of well-defined spiral arms or significant dust lanes, which further supports the classification as an elliptical galaxy. The color is generally redder, suggesting an older stellar population and a low star formation rate.
