The galaxy exhibits a morphology indicative of a potential ongoing or recent merger event. It presents as a disturbed system with two primary luminous cores or concentrations of light. One core is dominant, appearing brighter and more diffuse, potentially the main galactic nucleus. The second core is less prominent but distinctly visible with a more condensed or point-like appearance and a reddish hue. A faint bridge of light or tidal tail structure is observed between the two cores, suggesting gravitational interaction and material exchange. The overall shape deviates significantly from a regular elliptical or spiral form; instead, the galaxy presents with an irregular profile and elongated shape. There appear to be hints of faint tidal features or extended halos surrounding the main body of the galaxy, although the signal is weak. The color profile of the galaxy appears to be a blend of yellow and white light, with variations across the body of the galaxy. The redshift suggest that this is a massive galaxy with active star formation.
