This galaxy exhibits a distinct spiral structure, characterized by loosely wound arms. The arm count appears to be dominated by two major arms. A central bulge is present but it is not the dominant feature of this galaxy, with its brightness more evenly distributed across the disk. The galaxy is actively undergoing a merger, as evidenced by the highly disturbed morphology and interaction with another galactic body. The disruption to the spiral arm structure indicates a strong gravitational interaction. Tidal tails appear to be present, extending from the galaxy's main body, further supporting the interpretation of an ongoing merger event. Star formation may be elevated in some regions based on color, though the exact rate would require further spectral analysis. 
