  We demonstrate that the anisotropic stress-energy supporting the Kiselev
black hole can be mimicked by being split into a perfect fluid component plus
either an electromagnetic component or a scalar field component, thereby
quantifying the precise extent to which the Kiselev black hole fails to
represent a perfect fluid spacetime. The perfect fluid component carries either
an electric or a scalar charge, which then generates anisotropic
electromagnetic or scalar fields. This in turn generates anisotropic
contributions to the stress-energy. These in turn induce forces which partially
(in addition to the fluid pressure gradient) support the matter content against
gravity. This decomposition is carried out both for the original 1-component
Kiselev black hole and for the generalized N-component Kiselev black holes. We
also comment on the presence of energy condition violations (specifically for
the null energy condition --- NEC) for certain sub-classes of Kiselev black
holes.
