  Among the higher curvature gravities, the most extensively studied theory is
the so-called Einstein-Gauss-Bonnet (EGB) gravity, whose Lagrangian contains
Einstein term with the GB combination of quadratic curvature terms, and the GB
term yields nontrivial gravitational dynamics in $ D\geq5$. Recently there has
been a surge of interest in regularizing, a $ D \to 4 $ limit of, the EGB
gravity, and the resulting regularized $4D$ EGB gravity valid in $4D$. We
consider gravitational lensing by Charged black holes in the $4D$ EGB gravity
theory to calculate the light deflection coefficients in strong-field limits
$\bar{a}$ and $\bar{b}$, while the former increases with increasing GB
parameter $\alpha$ and charge $q$, later decrease. We also find a decrease in
the deflection angle $\alpha_D$, angular position $\theta_{\infty}$ decreases
more slowly and impact parameter for photon orbits $u_{m}$ more quickly, but
angular separation $s$ increases more rapidly with $\alpha$ and charge $q$. We
compare our results with those for analogous black holes in General Relativity
(GR) and also the formalism is applied to discuss the astrophysical
consequences in the case of the supermassive black holes Sgr A* and M87*.
