Observed is a galaxy displaying evidence of an ongoing interaction or merger. Two distinct, bright nuclei are visible, each surrounded by a diffuse halo of light. The upper nucleus appears slightly more compact and potentially brighter than the lower nucleus. The overall color appears to be blue-white suggesting a population of younger stars. There is some indication of tidal features or distortions, potentially faint wisps or tails, extending outward from the main body of the galaxy. The morphology deviates significantly from a smooth elliptical or a well-defined spiral structure, indicating dynamical disturbance. Based on visual assessment, it is likely that this system is undergoing significant gravitational interaction.
