The galaxy exhibits a disturbed morphology, indicative of possible interactions or a merger event. There is no definitive disk structure, and the overall form appears irregular. Patches of red are seen, potentially indicating regions of dust obscuration or areas of intense star formation. The central region appears brighter and more concentrated, possibly hosting an older stellar population. The galaxy extends relatively far, suggesting a substantial physical size. Evidence for ongoing star formation is present, though the overall colour suggests the object contains a considerable population of older stars. The smooth components account for a significant portion of the galaxy's light, but not a majority.
