  Following the interpretation of matter source that the energy-momentum tensor
of anisotropic fluid can be dealt with effectively as the energy-momentum
tensor of perfect fluid plus linear (Maxwell) electromagnetic field, we obtain
the regular higher-dimensional Reissner-Nordstr\"{o}m (Tangherlini-RN) solution
by starting with the noncommutative geometry inspired Schwarzschild solution.
Using the boundary conditions that connect the noncommutative Schwarzschild
solution in the interior of the charged perfect fluid sphere to the
Tangherlini-RN solution in the exterior of the sphere, we find that the
interior structure can be reflected by the exterior parameter, the
charge-to-mass ratio. Moreover, we investigate the stability of the boundary
under mass perturbation and indicate that the new interpretation imposes a
rigid restriction upon the charge-to-mass ratio. This restriction, in turn,
permits a stable noncommutative black hole only in the 4-dimensional spacetime.
