The galaxy appears to be undergoing a merging event. There is a central, roughly spherical, bright component. This component exhibits a smooth light distribution with a yellow-white hue, indicating an older stellar population. Adjacent to this main component is a more diffuse, elongated feature, suggestive of a disk or tidal tail. This second component exhibits a somewhat bluer color, potentially indicating younger stars within a disk system.

The merging appears to be in a late stage, due to the presence of a central bulge and a tidal tail. The galaxy is not a complete disk or spheroid galaxy, indicative of interaction. There is a slight irregularity observed in the disk-like feature, which may suggest gravitational disturbances due to the ongoing merging. The image suggests a complex morphology resulting from the interaction of two or more galactic components.
