The galaxy presents a moderately inclined disk structure. Evidence of spiral arms are present, though not sharply defined, appearing somewhat flocculent in nature. There is an indication of a central bulge, although it does not appear to dominate the overall structure. Star formation is active in the disk, as indicated by the presence of several blue regions suggestive of hot, young stars. A portion of the galaxy shows signs of disruption and possibly ongoing interaction with a companion galaxy. There is no obvious strong bar feature crossing the nucleus. The overall morphology indicates a galaxy undergoing active evolution, possibly through internal processes or external interactions.
