The galaxy appears to be undergoing a significant interaction or merger event. There are at least two distinct, bright nuclei visible, suggesting two progenitor galaxies are in the process of combining. The system has an irregular morphology, lacking a defined spiral or elliptical structure, and a substantial amount of tidal disruption or distortion is evident in the distribution of stellar material around the main bodies. The galaxy exhibits a range of colors across its structure. There is evidence of on-going star formation with relatively blue areas. Much of the galaxy has a yellowish hue, indicating the presence of an older stellar population. Overall, the appearance of this galaxy points towards an active, dynamic system with ongoing morphological transformation.
