  In this paper, we study the deflection of light by a class of charged
wormholes within the context of the Einstein-Maxwell-dilaton theory. The
primordial wormholes are predicted to exist in the early universe, where
inflation driven by the dilaton field. We perform our analysis through optical
geometry using the Gibbons-Werner method (GW), by adopting the Gauss-Bonnet
theorem and the standard geodesics approach. We report an interesting result
for the deflection angle in leading-order terms--namely, the deflection angle
increases due to the electric charge $Q$ and the magnetic charge $P$, whereas
it decreases due to the dilaton charge $\Sigma$. Finally, we confirm our
findings by means of geodesics equations. Our computations show that the GW
method gives an exact result in leading order terms.
