  In this article, we study regular scale-dependent black holes as
gravitational lenses. We obtain the deflection angle in the strong deflection
limit, from which we calculate the positions and the magnifications of the
relativistic images. We compare our results with those corresponding to the
Schwarzschild spacetime, and as an example, we apply and discuss these results
to the particular case of the supermassive black hole at the center of our
galaxy.
