The galaxy presents a primarily smooth morphology. The central region is bright and concentrated, indicating a prominent bulge. There is an extended, fainter disk component with an irregular shape. Evident is a possible tidal tail to the left of the main galaxy body, suggesting gravitational interaction or past merger activity, although the general consensus is that the galaxy is smooth. The system exhibits a range of colors, with a bluer region possibly indicating recent star formation. Overall, the galaxy appears to be a disk galaxy undergoing some form of disturbance.
