The galaxy appears to be in the late stages of a major merger. It exhibits a disturbed morphology, with two distinct nuclei, one slightly more diffuse than the other. There appears to be tidal tails or bridges of stellar material connecting the two nuclei, suggesting a strong gravitational interaction. The overall color is yellowish-white, potentially indicating a mix of stellar populations, including older stars and some ongoing star formation. The galaxy is moderately luminous and is not perfectly circular, more elliptical in shape.
