The galaxy exhibits a complex morphology, suggesting an ongoing or recent merger event. Two distinct, bright nuclei are visible, connected by a fainter bridge of stellar material. The overall shape deviates significantly from a regular elliptical or spiral form. The color gradient across the galaxy indicates variations in stellar populations or dust content. The nuclei appear yellowish-white, possibly indicating older stellar populations, while the bridge exhibits a slightly bluer hue. There is evidence of significant tidal disruption, with extended faint features surrounding the main body of the galaxy, which may indicate tidal tails. The system has moderate luminosity.
