We analytically prove the linear radial stability of non-Abelian black holes with quartic self-interactions. The background, constructed from the Wu–Yang magnetic monopole ansatz, is an exact black-hole solution carrying a non-Abelian magnetic charge controlled by a single coupling parameter , and admits two distinct branches. The odd sector is always stable, while in the even sector the effective potential is positive for branch~I and negative for branch~II, establishing stability and potential instability, respectively. The potential instability of branch~II is consistent with its connection to the perturbatively unstable Einstein–Yang–Mills Reissner–Nordström solution. Branch~I remains linearly stable throughout the physical domain of where the solutions are regular and free of naked singularities. Our results prove the existence of the first linearly stable asymptotically flat hairy black holes in four dimensions with a minimally coupled non-Abelian Proca self-interaction.

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