The galaxy presents a somewhat irregular morphology, displaying features indicative of an ongoing or recent merger event. A prominent disk component is visible, though it exhibits a warped and distorted structure. Evident within the disk are spiral arm segments, though their definition is disrupted, suggesting tidal interactions. A noticeable bar structure is present, appearing moderate in strength. The bulge of the galaxy appears to be of moderate size relative to the disk. The overall color suggests active star formation occurring, particularly along the fragmented spiral arms and in clumpy regions within the disk. There is a secondary object close to the galaxy which could be part of the system. There is evidence of a strong disturbance as the shape of the galaxy is not uniform.
