The galaxy exhibits a clear disk-like structure, viewed at an angle that is neither perfectly face-on nor edge-on. Distinct spiral arms are apparent, displaying a loosely wound morphology. Two spiral arms are clearly visible, and they appear to have a flocculent nature.

The central bulge is small compared to the disk's size, with a smooth appearance. There is a prominent central bar.

There is an object causing a major disturbance to the galaxy's morphology, implying a strong gravitational interaction and/or tidal forces. The galaxy appears to be undergoing a major merger.
