We study the dynamics of dark energy in the presence of a 2-form field coupled to a canonical scalar field \phi .
We consider the coupling proportional to e ^ { - \mu \phi / M _ { pl } } H _ { \alpha \beta \gamma } H ^ { \alpha \beta \gamma } and the scalar potential V ( \phi ) \propto e ^ { - \lambda \phi / M _ { pl } } , where H _ { \alpha \beta \gamma } is the 2-form field strength , \mu, \lambda are constants , and M _ { pl } is the reduced Planck mass .
We show the existence of an anisotropic matter-dominated scaling solution followed by a stable accelerated fixed point with a non-vanishing shear .
Even if \lambda \geq { \cal O } ( 1 ) , it is possible to realize the dark energy equation of state w _ { DE } close to -1 at low redshifts for \mu \gg \lambda .
The existence of anisotropic hair and the oscillating behavior of w _ { DE } are key features for distinguishing our scenario from other dark energy models like quintessence .