  We find that the four dimensional cosmological Einstein-Yang-Mills theory
with $SU(2)$ gauge group admits Lifshitz spacetime as a base solution for the
dynamical exponent $z>1$. Motivated by this, we next demonstrate numerically
that the field equations admit black hole solutions which behave regularly on
the horizon and at spatial infinity for different horizon topologies. The
solutions depend on one parameter, the strength of the gauge field at the
horizon, which is fine-tuned to capture the Lifshitz asymptotics at infinity.
We also discuss the behavior of solutions and the change in Hawking temperature
for black holes that are large or small with respect to the length scale $L$,
which is itself fixed by the value of the cosmological constant.
