The galaxy presents a generally smooth and rounded morphology. Its light is centrally concentrated, exhibiting a yellowish-white hue that transitions into a redder, fainter outer region. There is no clear indication of spiral arms or a prominent disk structure. Slight irregularities in the outer regions may hint at minor disturbances or ongoing interactions. The overall structure suggests a relatively evolved system, possibly an elliptical galaxy. The lack of prominent blue regions indicates relatively low current star formation activity.
