This galaxy exhibits a morphology indicative of a system undergoing a major merger. The light distribution is relatively smooth but highly disturbed, with two distinct bright cores visible. The overall shape appears elongated. The system displays a yellow-red color, suggesting an older stellar population is dominant. The color distribution is fairly uniform, without strong gradients, which may indicate that star formation is suppressed overall in the system, or has ended in one core, but continues in the other. The merging process has resulted in a significant deviation from a regular elliptical or disk galaxy, and it is likely that tidal features or extended stellar halos are present, though not discernible with the image quality provided.
