  In this paper an intrinsically non-Abelian black hole solution for the SU(2)
Einstein-Yang-Mills theory in four dimensions is constructed. The gauge field
of this solution has the form of a meron whereas the metric is the one of a
Reissner-Nordstr\"om black hole in which, however, the coefficient of the
$1/r^2$ term is not an integration constant. Even if the stress-energy tensor
of the Yang-Mills field is spherically symmetric, the field strength of the
Yang-Mills field itself is not. A remarkable consequence of this fact, which
allows to distinguish the present solution from essentially Abelian
configurations, is the Jackiw, Rebbi, Hasenfratz, 't Hooft mechanism according
to which excitations of bosonic fields moving in the background of a gauge
field with this characteristic behave as Fermionic degrees of freedom.
