The Hamiltonian analysis for f(T) gravity implies the existence of at least one
scalar-type degree of freedom (DoF). However, this scalar DoF of f(T) gravity does not manifest
in linear perturbations around a cosmological background, which indicates an underlying strong
coupling problem. In this work we expand the scope by introducing an extra scalar field
non-minimally coupled to f(T) gravity, aiming to address or alleviate the aforementioned strong
coupling problem. Employing the effective field theory (EFT) approach, we provide a class of
torsional EFT forms up to second order operators, avoiding the Ostrogradsky ghost. To illustrate
this phenomenon, we study a simple model and perform a detailed analysis of its linear scalar
perturbations. The results demonstrate that the coupling terms in this toy model are necessary to
avoid the initial degenerate situation. The complete avoidance of new constraints requires more
coupling terms. Once this vanishing scalar DoF starts propagating in cosmological background at
linear level, this phenomenon will demand a revisit of the strong coupling issue that arises in
f(T) gravity, particularly in the presence of matter coupling.