  We derive and investigate the physical properties of asymptotically flat
noncommutative regular charged black holes with a Gaussian mass density
distribution and a Weibull electric charge density distribution. Both
distributions replace the Dirac one and introduce a set of substitution rules
constituting new ways of counting. The solutions have a de Sitter behavior in
the vicinity of the origin provided the electric charge density is Weibull of
the form $r^{n/2}{\rm e}^{-r^2/(4\theta^2)}$ with $n\geq 1$. The electric field
and temperature are finite for all values of the radial coordinate, mass, and
charge. The charge is bounded from above for stability reasons and stable
charged quantum particles have mass and charge bounded from below and from
above within the simplified semi-classical model we present in this work.
