  In this work, the Ellis drainhole solution is derived in Einstein-{\AE}ther
gravity, and subsequently, the axial quasinormal modes of the resulting
drainhole are investigated. Owing to the presence of a minimally coupled scalar
field with antiorthodox coupling polarity, the resultant metric solution is
featured by a throat instead of a horizon, for which static {\ae}ther solution
becomes feasible. Moreover, the derived master equations for the axial
gravitational perturbations consist of two coupled vector degrees of freedom.
By utilizing the finite difference method, the temporal profiles of the
quasinormal oscillations are evaluated, and, subsequently, the complex
frequencies are extracted and compared against the specific values obtained by
the WKB method when the coupling is turned off. Besides, the effect of the
coupling on the low-lying quasinormal spectrum is explored, and its possible
physical relevance is discussed.
