This galaxy appears to be undergoing a significant interaction or merging event. There is noticeable distortion in its overall structure. A diffuse, extended halo of light surrounds a more concentrated central region. Within the central region, there is evidence of multiple nuclei or bright clumps, indicative of a possible merger in progress. The main body displays a flattened, disk-like component. The disk has a clumpy structure with potential spiral arm segments, but these are highly disrupted. Patches of blueish light are interspersed with redder regions, suggesting a mix of both older stellar populations and ongoing star formation. The galaxy exhibits tidal tails and other disturbed morphological features, pointing towards gravitational interactions. The overall shape is irregular and asymmetrical, deviating significantly from a typical spiral or elliptical morphology.
