  In the present paper, we investigate wormholes in 4D-Einstein-Gauss-Bonnet
gravity without the requirement of exotic matters. We have taken the radial
dependent red-shift function $\phi=\ln \left( {\frac {r_{{0}}}{r}}+1 \right)$
and shape function $b(r)={\frac{r_{0}\ln(r+1)}{\ln({r_0}+1)}}$ as well as
anisotropic matter sources through equation of state (EoS) $p_r(r) = \omega
\rho(r)$. We examine the energy conditions, flaring out condition, throat
condition and anisotropic parameter. The volume integral quantifier is also
analyzed to validate the existence and stability of the WH solution. We find,
for -ve branch wormhole solutions satisfy the null energy conditions (NEC)
throughout the entire space time and +ve branch reduces exactly to
Morris-Thorne of GR.
