This galaxy presents as a disturbed spiral, undergoing a significant interaction or merger. The morphology appears irregular, deviating from a classic spiral structure. There are extensive, diffuse features evident, indicative of tidal forces at play. Faint spiral arms are visible, displaying a medium to tight winding, disrupted by the ongoing interaction. A subtle bar structure may be present, though it's obscured by the disruption. The central bulge is ill-defined, appearing small to moderately sized relative to the overall disk. There are no features to support that this galaxy is smooth. Evidence of merging is apparent, possibly with a smaller galaxy. It is difficult to resolve distinct regions of star formation. There appears to be a lot of dust within the galaxy, evidenced by patchy regions of extinction in the galaxy. The core appears to be actively undergoing change.
