This galaxy appears to be a spiral galaxy, exhibiting significant distortions in its morphology. The spiral arms are well-defined and prominent, showing a distinct winding pattern that appears to be medium, transitioning from tight in some areas to loose in others. Evidence suggests it may have 2-3 arms. The galaxy's bulge is relatively small and less prominent, with a moderate contribution to the overall light distribution. There seems to be a bar structure. Overall, the galaxy displays signatures of a recent interaction or merger event, disrupting the disk and potentially stimulating star formation.
