The observed galaxy presents as a luminous, interacting system. It exhibits a complex morphology indicative of an ongoing merger event. Two distinct nuclei are observed, one brighter and more compact than the other. The overall shape appears distorted from a regular elliptical or spiral form. A tidal tail or bridge of material extends between the two nuclei, suggesting strong gravitational interaction. The color gradient shows a central yellowish-white hue transitioning to a slightly bluer outer region, possibly indicating varying stellar populations or dust obscuration. There is evidence of disturbance throughout the disk and halo.
