The galaxy exhibits a morphology indicative of a merger event. Evident are two distinct luminous clumps, potentially representing the cores of the merging galaxies, with a diffuse, disturbed halo surrounding the system. There is extended tidal structure indicative of an interaction. The system displays a color gradient, transitioning from bluer regions within the core area to redder hues in the outer reaches. The overall color suggests a population of older stars and potentially ongoing star formation within the interacting cores.
