This galaxy appears to be undergoing a significant interaction or merger. It has a disturbed morphology, with a bright, central region and extended tidal features or distorted arms. There are two distinct bright knots visible, potentially representing the cores of the original galaxies or regions of intense star formation triggered by the interaction. The overall color suggests a mix of stellar populations. The presence of bluer hues in some areas could indicate ongoing star formation, while yellower/redder regions suggest older stellar populations.
