The galaxy presents a predominantly smooth morphology, exhibiting characteristics of an elliptical or lenticular type. The light distribution appears centrally concentrated, with a gradual decrease in intensity towards the outer regions. There is a clear elongation, indicating a departure from perfect circularity. The galaxy exhibits a reddish-yellow hue, suggestive of an older stellar population dominated by evolved stars. There is no obvious indication of spiral arms or significant dust lanes. The overall structure seems relatively undisturbed, lacking evidence of major mergers or strong tidal interactions. The galaxy is not perfectly round, but appears oblong in its overall shape, being more cigar-shaped than round.
