  In the present work, we {study} static spherically symmetric solutions
representing wormhole configurations in Poincar\`{e} gauge theory ({{\sf
PGT}}). The gravitational sector of the Lagrangian is chosen as a subclass of
{\sf PGT} Lagrangians for which, the spin-$0^+$ is the only propagating torsion
mode. The spacetime torsion in {\sf PGT} has a dynamical nature even in the
absence of intrinsic angular momentum (spin) of matter, hence, {torsion can
play a principal role in the case of usual spin-less gravitating systems. We
therefore} consider a spin-less matter distribution with an anisotropic energy
momentum tensor ({\sf EMT}) as the supporting source for wormhole structure {to
obtain a class of zero tidal force wormhole solutions.} It is seen that the
matter distribution obeys the physical reasonability conditions, i.e., the weak
({\sf WEC}) and null ({\sf NEC}) energy conditions either at the throat and
throughout the spacetime. We further consider varying equations of state in
radial and tangential directions via definitions $w_r(r)=p_r(r)/\rho(r)$ and
$w_t(r)=p_t(r)/\rho(r)$ and {investigate} the behavior of state parameters {at
the throat of wormhole}. We observe that our solutions allow for wormhole
configurations without the need of exotic matter. Observational features of the
wormhole solutions are also discussed utilizing gravitational lensing effects.
It is found that the light deflection angle diverges at the throat (which
indeed, effectively acts as a photon sphere) and can get zero and negative
values depending on the model parameters.
