The galaxy presents a complex morphology, suggesting an ongoing or recent interaction. It appears to be composed of at least two distinct components. A dominant, relatively smooth, and roundish component is apparent, showing a concentration of light towards the center and a gradual decline in intensity outwards. 

A secondary component seems to be interacting with the primary one. This is inferred by a bridge of luminous material or a tidal tail extending outwards from the main body. The structure has a fuzzy or diffuse appearance. Some level of disturbance is evident in the system's overall structure, likely caused by gravitational interactions.
