The galaxy appears to be undergoing a merger or a significant interaction with a companion galaxy. The primary galaxy exhibits a somewhat elliptical morphology with a smooth central bulge that is slightly elongated, and a hint of disk-like structure. The colour of this primary component indicates a relatively older stellar population. 

A smaller, adjacent companion galaxy shows a distinctly bluer hue, which suggests ongoing or recent star formation. The morphology of the companion is less defined, possibly disrupted by tidal forces from the interaction. It is located on the outskirts of the main galaxy.

There is a bridge of material or a tidal tail connecting the two galaxies, though the precise composition of this bridge is not readily determined from this image alone. The overall disturbance in morphology points towards a dynamic interaction between the two galaxies.
