This galaxy presents as a spiral type, exhibiting a distinct disk-like structure. The spiral arms are prominent and appear loosely wound, suggesting a later Hubble type classification. Two major arms are clearly visible, originating from a central bulge. The bulge itself seems relatively small. It appears there may be a bar-like structure extending from the bulge, which may indicate a barred spiral morphology. The galaxy shows signs of an interaction or merger, indicated by tidal tails. One tail is especially strong and is significantly disrupting the galaxy. The presence of the tidal tail may indicate an ongoing or recent merger event, potentially with another galaxy that is now fully merged with the primary galaxy. The galaxy exhibits a blue color, indicative of recent star formation. This, combined with the distorted morphology, further strengthens the interpretation of an interaction or merger event.
