The galaxy presents a morphology indicative of a disturbed system, possibly undergoing a merging event. The galaxy exhibits an elongated form, with a noticeable asymmetry in its distribution of light. There is a distinct feature which is likely tidal debris. The distribution of light within the galaxy shows a complex structure. Some regions appear relatively smooth, while others show clumpy distributions. Patches of blue light suggest regions of active star formation. Overall, the galaxy's morphology appears irregular and chaotic, suggesting ongoing gravitational interactions with another galaxy or a recent merger event.
