The galaxy presents as a complex system, likely undergoing a significant interaction or merger event. Two distinct nuclei are visible, each associated with a stellar component. These components appear somewhat distorted, suggesting gravitational disruption. A tenuous bridge of light connects these two main bodies, indicating tidal interactions and possible material transfer between them. The overall morphology leans towards being smooth, with a slight indication of a disk-like structure emerging. A minor disturbance can be seen in the form of asymmetry of the arms. The galaxy exhibits a moderate level of star formation activity, with some regions appearing slightly bluer than others. The shape of the galaxy is somewhere between round and elliptical, and appears somewhat distorted. There are no nearby major merger indications.
