The object appears to be an interacting galaxy system or a galaxy undergoing a significant tidal disruption. There are two primary, relatively concentrated luminous regions, suggestive of galactic nuclei. These regions exhibit a yellowish hue. A faint, diffuse tidal tail-like structure connects these two brighter components, displaying a more reddish tint. This suggests potentially older stellar populations within the tail. The overall morphology indicates a post-merger or ongoing interaction. Based on the red shift, this is a galaxy system from the distant universe. Further spectroscopic analysis would be beneficial to determine the stellar populations and gas dynamics within the system.
