The galaxy presents a disturbed morphology, suggesting possible ongoing or recent interaction. It appears to be a spiral galaxy with a notable disk structure.

The spiral arms are clumpy and ill-defined. There appear to be many HII regions within the spiral arms. The spiral arms also have a somewhat flocculent structure. The galaxy exhibits a moderate central bulge, with a bar-like feature possibly present. The disk extends beyond the central bulge, indicating a developed structure. Some regions show evidence of possible star formation with bluer colors. There appear to be possible tidal tails present indicating an ongoing merger.