The galaxy exhibits a faint, diffuse morphology. No distinct spiral arms or a prominent central bulge are discernible. It appears roughly circular in shape, lacking any obvious asymmetries or tidal features suggestive of a recent major merger. The light distribution is relatively uniform across the visible extent of the object. There may be evidence of minor disturbances. The lack of clear structure suggests that it might be a smooth elliptical galaxy. The absence of a redder color in the central regions might suggest a lack of older stars or a significant amount of dust obscuration.
