The object appears to be a single galaxy undergoing a significant merger or interaction with another galaxy or smaller object. The main body of the galaxy exhibits a disturbed morphology, showing a mixture of smooth and irregular features, indicating ongoing tidal forces reshaping its structure. Distinct color variations are evident across the galaxy. There is a blueish hue in certain areas, which could represent a higher amount of new star formation, a yellow-white region and even redder areas, which suggest a older stellar population or dust obscuration. This color heterogeneity supports the idea of merging. An irregular shape with hints of multiple nuclei reinforces the hypothesis of an ongoing merger.
