The object presents as a disturbed galaxy system, likely in the late stages of a merger. Two distinct nuclei are visible, one exhibiting a yellowish-white hue and the other displaying a more orange-red coloration. There is evidence of tidal features between the two nuclei suggesting gravitational interaction. The overall shape deviates significantly from a standard elliptical or spiral morphology, indicating ongoing disruption. While some smoothness is observed in the light distribution, the prevailing impression is that of a dynamically active system.
