The galaxy appears to be a relatively smooth, elliptical or lenticular system, with a centrally concentrated bulge that dominates the overall light distribution. The bulge exhibits a yellowish-red hue, suggesting an older stellar population with reduced ongoing star formation. The outer regions appear more diffuse, with the overall shape being in between a perfect circle and a cigar shape. There is a possible indication of a slight tidal disturbance, although the system generally exhibits characteristics consistent with a relaxed morphology and minimal ongoing or recent merging activity.
