The object appears as a merging system comprised of two distinct, relatively spherical concentrations of luminous material. The overall color profile is predominantly yellow-orange, suggesting a population of older stars and/or dust obscuration. There is a subtle color gradient, with the central regions of each concentration trending towards a slightly redder hue. Both concentrations show relatively smooth luminosity profiles, with no apparent spiral arm structures or prominent dust lanes visible. Given the lack of clear morphological features beyond the two primary components and a slightly disturbed form, this system is likely undergoing a late stage merger. Star formation activity appears to be suppressed based on the color, suggesting most of the gas has been consumed or expelled.
