This galaxy appears to be undergoing a significant interaction or merger. It presents a morphology that deviates from a standard elliptical or spiral form. The light distribution is complex and not smoothly distributed. There appear to be two distinct, bright concentrations of light suggesting two galactic cores, with some tidal features or extended material connecting them. These concentrations are roughly spherical but with some visible elongation. The overall color suggests an older stellar population, with a redder hue dominating. There may be some indication of disturbed dust lanes or tidal tails indicative of ongoing gravitational interaction, and there is evidence that a significant amount of merging is likely happening, with the galaxy being in between a smooth and merging shape.
