  We use Einstein, Landau-Lifshitz, Papapetrou and Weinberg energy-momentum
complexes to evaluate energy distribution of a regular black hole. It is shown
that for a regular black hole, these energy-momentum complexes give the same
energy distribution. This supports Cooperstock hypothesis and also
Aguirregabbiria et al. conclusions. Further, we evaluate energy distribution
using M$\ddot{o}$ller's prescription. This does not exactly coincide with ELLPW
energy expression but, at large distances, they become same.
