The galaxy presents as a disturbed system, likely undergoing a major merger event. Two distinct, bright, and concentrated areas are visible, presumably the cores of the merging galaxies. These cores exhibit a yellowish-orange hue, suggestive of an older stellar population and potentially significant dust obscuration. Faint tidal tails or streams of material extend outwards from the main body of the galaxy, indicating gravitational interactions. There is faint bluer emission observed, which might indicate regions of active star formation, particularly in the outer regions of the galaxy.
