  In this work, we investigate the gravitational lensing of a charged black
hole (spherically symmetric) within the context of Lorentz violation triggered
by an antisymmetric tensor field. Our calculations consider two different
scenarios: the weak and strong deflection limits. For the weak deflection
limit, we employ the Gauss-Bonnet theorem to obtain our results. In the strong
deflection limit, we utilize the Tsukamoto methodology, which provides
measurable outcomes such as relativistic image positions and magnifications.
Applying the latter methodology, we analyze the gravitational lensing by
Sagittarius $A^{*}$ and derive the related observables, which are expressed as
functions of the Lorentz violation parameter. Finally, the time delay is
addrressed as well.
