  In this work, we study the gravitational lensing by a Lorentz-violating (LV)
black hole inspired by the recent contribution [1]. Explicitly, we concentrate
on a specific application: we perform the computation of gravitational lensing
effects under the strong field limit. In particular, we analytically derive the
deflection angle so that the lens equation can also be addressed. This
methodological approach yields physically measurable outcomes, including the
determination of relativistic image positions and their corresponding
magnifications. As an application of this methodology, we consider the
gravitational lensing by Sagittarius A${}^*$ and obtain the corresponding
observables expressed as functions of the LV parameter.
