This galaxy appears to be undergoing a significant merger. It is composed of two distinct components or galactic cores, each with a relatively smooth morphology. The upper core is slightly more circular, while the lower core appears marginally elongated. There is evidence of tidal interactions between the two cores in the form of faint, diffuse light extending outwards. These structures exhibit a bluer color, suggesting recent or ongoing star formation in these areas. The redder central regions of each core indicate a higher concentration of older stellar populations. The system as a whole exhibits moderate luminosity. The overall structure suggests a system in the late stages of a merger.
