  The quasinormal modes (QNMs) of a regular black hole with charge are
calculated in the eikonal approximation. In the eikonal limit the QNMs of black
hole are determined by the parameters of the unstable circular null geodesics.
The behaviors of QNMs are compared with QNMs of Reisner-Nordstr\"{o}m black
hole, it is done by fixing some of the parameters that characterize the black
holes and varying another. We observed that the parameter that is related one
effective cosmological constant at small distances , determines the behaviors
of the QNMs of regular black hole with charge.
