The galaxy exhibits a relatively small angular size. Morphologically, it appears to be a disk galaxy viewed at a high inclination, close to edge-on. The central bulge is bright and concentrated, showing a slight yellow tinge. The disk itself presents a blue-green hue, suggesting the presence of ongoing star formation. There is evidence of some minor disturbances or asymmetries in the disk, and it is possibly interacting with another galaxy. It cannot be ruled out that it is a single galaxy that is heavily distorted. There are tidal tails extending from both galaxies/parts of the galaxy.