  We find the most general spherically symmetric non singular black hole
solution in a special class of teleparallel theory of gravitation. If $r$ is
large enough, the general solution coincides with the Schwarzschild solution.
Whereas, if $r$ is small, the general solution behaves in a manner similar to
that of de Sitter solution. Otherwise it describes a spherically symmetric
black hole singularity free everywhere. Moreover, the energy associated with
the general solution is calculated using the superpotential given by M{\o}ller
1978.
