The galaxy presents a morphology that appears to be neither purely elliptical nor a well-defined spiral. It exhibits a centrally concentrated bulge that is bright and yellowish. The outer regions show some disk-like features, with a hint of spiral arm structure. There is a mixture of bluer regions suggestive of ongoing star formation and yellower areas, which suggest an older stellar population. The galaxy appears to be undergoing some form of interaction or disturbance, with a slightly irregular shape. A small fraction of the galaxy shows signs of disturbance, but the overall shape doesn't look like it is undergoing a major merger.
