The galaxy exhibits a morphology characterized by a central, relatively smooth bulge with some indication of a disrupted disk structure. There may be a merging event occuring. The galaxy appears to be actively forming stars, particularly within the features of its disk, which are more prominent along one side of the galaxy than the other. This asymmetry could be indicative of ongoing interactions or recent accretion events. The central region shows evidence of older stellar populations, suggesting a history of prior star formation. The overall color profile indicates a mix of stellar populations, with bluer regions associated with younger stars and redder regions with older stars. There appears to be some tidal disturbance of the galaxy, as evidenced by faint wisps or streams of light. The galaxy shows a combination of smooth and clumpy regions, contributing to an irregular morphology.
