The galaxy presents a complex morphology, exhibiting characteristics of both a disk galaxy and a possible interaction. Its central region is bright and concentrated, appearing yellowish-white, suggestive of an older stellar population. A flattened disk-like structure extends outwards from the core. Two distinct lobes, or plumes, of reddish color are located perpendicular to the plane of the disk, suggesting possible ejection or tidal features. They extend away from the galaxy, and are relatively small in size. Although the shape of the galaxy disk is fairly smooth, there might be some features that indicate some kind of disturbances. Based on its morphology, it is most likely that this galaxy is interacting with another galaxy. 
