The galaxy appears to be undergoing a significant merger event. Two distinct galactic nuclei are visible. One nucleus exhibits a smoother, more rounded morphology with a yellowish-orange hue. The other nucleus presents a bluer color, suggesting a younger stellar population or increased star formation. There are disturbances in the overall structure, likely due to the gravitational interactions between the merging galaxies. The system has an approximate effective radius of 5 kpc, indicative of a massive galaxy. The morphology indicates a possible elliptical galaxy. The estimated stellar mass indicates a large galaxy. The color suggests that the specific star formation rate is low in both galaxies.
