We present multi-epoch multi-frequency VLBI images of the compact polarized
radio structure of the quasar 4C 39.25. Between 1995 and 1999, the total i
ntensity images at 15, 22, and 43 GHz have remained almost unperturbed, whi
le there have been significant changes in the polarized intensity maps toge
ther with a related rotation of the polarization angle. These changes in th
e polarized structure trace in great detail the interaction between a movin
g and a standing component. We interpret the stationary feature as a bend i
n the jet trajectory in a plane that does not contain the observer, and the
moving one as a shock turning around the bend.