  A study about the energy and momentum distributions of a new charged regular
black hole solution with a nonlinear electrodynamics source is presented. The
energy and momentum are calculated using the Einstein and M{\o}ller
energy-momentum complexes. The results show that in both pseudotensorial
prescriptions the expressions for the energy of the gravitational background
depend on the mass $M$ and the charge $q$ of the black hole, an additional
factor $\beta $ coming from the spacetime metric considered, and the radial
coordinate $r$, while in both prescriptions all the momenta vanish. Further, it
is pointed out that in some limiting and particular cases the two complexes
yield the same expression for the energy distribution as that obtained in the
relevant literature for the Schwarzschild black hole solution.
