The galaxy exhibits a distinct disk morphology, though its classification is complicated by apparent interactions. A noticeable tidal tail extends outwards, displaying a gradient from warmer hues near the core to cooler tones. Within the primary disk structure, spiral arms are visible, though somewhat diffuse. The overall color suggests moderate levels of ongoing star formation activity within the disk and tail structures. There is a possible bar feature visible. The central bulge component appears small relative to the overall size of the galaxy, and it is not the dominant part of the visible galaxy. Evidence of a potential merger is visible due to distortions in the disk.
