The galaxy appears to be undergoing a significant interaction, possibly a merger. There are two distinct, bright nuclei visible, indicating two separate galactic centers in close proximity. These centers are roughly circular and exhibit a yellow-white hue. A fainter, more diffuse region of light extends between and beyond the two nuclei, suggesting tidal interactions and material exchange between the merging components. There is a hint of a disturbed morphology, suggesting a system that is far from a relaxed state. There may be some minor disturbances in the surrounding halo. The overall color appears to be trending towards the red end of the spectrum, which may indicate a population of older stars. More data is required to determine the full nature of this interaction.
