  We consider gravitational lensing under a weak-field approximation and in a
strong deflection limit by a Bronnikov-Kim wormhole with the same metric as the
one of a wormhole which has been suggested in Einstein-Dirac-Maxwell theory.
The metric approaches into the metric of an extreme charged
Reissner-Nordstr\"{o}m black hole in a black hole limit and it becomes the
metric of an spatial Schwarzschild wormhole in an ultrastatic limit. In both of
the black hole limit and the ultrastatic limit, the coefficient of a divergent
term and the constant term of the deflection angle of a light in the strong
deflection limit can be obtained exactly without expanding of parameters of the
spacetime. Interestingly, in the both limits to the black hole and the
ultrastatic wormhole, we obtain exactly the same coefficient and constant term
in the strong deflection limit.
