  We consider the properties of a static axially symmetric wormhole described
by an exact solution of Einstein's field equations and investigate how we can
distinguish such a hypothetical object from a black hole. To this aim, we
explore the motion of test particles and photons in the wormhole's space-time
and compare it with the particle dynamics in the well known space-times of
Schwarzschild and Kerr black holes. We show that precise simultaneous
measurement of test particle motion and photon motion may provide the means to
distinguish the wormhole geometry from that of a black hole.
