The galaxy presents as an elongated, potentially merging system. Two primary components are discernible, each appearing as a concentrated region of light. These are connected by a fainter, diffuse bridge of luminous material. The color profile shows a gradient, shifting from yellow-orange hues near the two main centers towards a bluer tint in the outer regions. The overall structure suggests ongoing gravitational interaction, possibly indicative of a galactic merger in progress. The system appears to be actively forming stars at a considerable rate. The estimated mass of the galaxy suggests it is a significant object. The morphology suggests a disk component exists, alongside a significant fraction of smooth components. The lack of strong tidal tails indicates the merger is likely in its later stages or involves galaxies of considerably different sizes.
