The galaxy appears to be in the process of merging or interacting with another galaxy. One component has a smooth, elongated shape while the other is more diffuse, with a less defined structure. The elongated component exhibits a redder hue, potentially indicating an older stellar population or significant dust obscuration. There is evidence of disruption or tidal features, suggesting gravitational interaction between the components. Overall, this galaxy is a system undergoing morphological transformation, with the potential for significant star formation activity related to this process.