The galaxy appears to be undergoing a major merger event. Two distinct galactic nuclei are observed. The larger galaxy presents a somewhat smooth but disturbed morphology, likely indicative of tidal interactions. Faint extensions or tidal tails are visible on one side, suggesting gravitational interactions between the two galaxies. The overall color profile of both galaxy components exhibits a gradient from a yellowish-white core towards a bluer outer halo. The disturbed morphology and color gradients suggest active star formation regions within the galaxy.
