The object appears to be a galaxy undergoing a merging event. Two distinct, but closely interacting, galactic nuclei are visible. The larger, primary nucleus exhibits a predominantly smooth morphology with a blue-white hue. The smaller, secondary nucleus is situated close to the primary and is characterized by a yellowish hue. There appears to be a gravitational disturbance present in the structure, as it does not feature spiral arms or bar features. Overall, the galaxy appears to be in an intermediate stage of merger, with strong interaction between the two galactic components, indicating ongoing star formation. The object's apparent roundness suggests it is not an edge-on disk galaxy.
