The galaxy exhibits a disturbed morphology, suggestive of an ongoing or recent merger event. There appear to be two distinct components. One of them shows spiral arm features. The spiral arms are not tightly wound. It is difficult to resolve the spiral arm count but there appear to be two to three discernible spiral arms. A relatively small bulge appears present. There also is an area of major disturbance. The color index is somewhat blue suggesting ongoing star formation. Overall this galaxy is most likely merging with another galaxy.
