The galaxy appears to be undergoing a significant interaction, potentially a merger. There are at least three distinct luminous components visible. One component, located to the west, exhibits a more diffuse morphology and a bluer color, possibly indicating active star formation regions. The two components to the east show a reddish hue, suggesting an older stellar population or higher dust content. The overall structure is disturbed, with possible tidal tails or bridges connecting the different components, although these are not very prominent. This distorted morphology is a common characteristic of galaxies experiencing mergers. The galaxy is of moderate size, with a likely stellar mass on the order of 10^10 solar masses. Star formation is ongoing, but not at an exceptionally high rate, indicating the galaxy is not a strong starburst system. The image suggests that the interaction is in relatively early stages, with the individual galaxies still distinguishable rather than completely coalesced.
