  Gauge-flation, inflation from non-Abelian gauge fields, was introduced in
[1,2]. In this work, we study the cosmic no-hair conjecture in gauge-flation.
Starting from Bianchi-type I cosmology and through analytic and numeric studies
we demonstrate that the isotropic FLRW inflation is an attractor of the
dynamics of the theory and that the anisotropies are damped within a few
e-folds, in accord with the cosmic no-hair conjecture.
