The galaxy appears to be an elliptical type, exhibiting a smooth, largely featureless morphology. The light distribution is centrally concentrated with a gradual decrease in intensity outwards. The color indices suggest a predominantly older stellar population, consistent with an elliptical classification. There is a secondary smaller galaxy also visible, it appears to be a disk galaxy. There may be some distortion of the larger galaxy caused by the smaller galaxy, though this is difficult to confirm without further spectral analysis. There appears to be minor disturbance of the larger galaxy.
