The galaxy appears to be a spiral galaxy undergoing a significant interaction or merger. The central bulge region is moderately sized and shows a relatively smooth appearance, suggesting an older stellar population. Emerging from the central region, there are indications of faint, disturbed spiral arms. These arms appear to be disrupted, possibly due to tidal forces associated with the interaction. There's no strong central bar structure visible, but the overall morphology shows features that would be classified as disturbed. There's no clear evidence of a pronounced dust lane. Star formation seems to be ongoing, though it seems more moderate than vigorous, this is inferred from the subtle color variations. The tidal features suggest a relatively recent interaction, implying heightened star formation activity in the past.
