The galaxy presents a morphology characteristic of a spiral galaxy undergoing a significant interaction. The central bulge appears prominent and moderately sized, exhibiting a yellowish hue, possibly indicating an older stellar population. Spiral arms are present, though somewhat disrupted, displaying segments of blue which suggests areas of active star formation. Extensive regions are exhibiting signs of tidal disruption, with distorted outer arms. The overall structure is complex and asymmetrical, which indicates a current or recent merger event. There appear to be multiple tidal tails or bridges extending outward, evidence of gravitational interaction with a nearby galaxy. There is also a patch of reddish dust in the galaxy near the central bulge. The presence of blue regions suggests ongoing star formation despite the interaction.
