The galaxy presents as an apparent merger, exhibiting a complex morphology. Two primary galactic bodies are distinguishable, with the larger exhibiting a smooth, elliptical-like profile and a yellowish hue, indicative of an older stellar population. This component appears relatively undisturbed. The smaller, secondary body displays a more irregular shape and a bluer color, suggesting more recent or ongoing star formation. There are hints of tidal features or distortions present, possibly indicative of gravitational interactions between the two galaxies. The system is relatively compact, suggesting that the merger event is in its later stages, though it is hard to tell.
