The galaxy presents a complex morphology, appearing disturbed and possibly undergoing a merging event. There is evidence of tidal features, with faint extensions or tails visible. The central region shows a concentration of light with a clumpy structure. Patches of bluer light are evident towards the center, while outer regions exhibit a redder hue. The galaxy's overall shape deviates significantly from a smooth elliptical or well-defined spiral structure, indicating gravitational interactions are actively disrupting its form.
