  We compute the shadow cast by a charged Morris-Thorne wormhole when the light
source is a star located beyond the mouth which is opposite to the observer.
First, we provide an extensive analysis of the geodesic properties of the
spacetime, both for null and massive particles. The geometrical properties of
this solution are such that independently of the viewing angle, some light rays
always reach the observer. Additionally, the structure of the images is
preserved among the different values of the charge and scales proportionally to
the charge value.
