  In this research work, our primary focus revolves around the examination of a
specific category of traversable wormholes known as topologically charged
generalized Schwarzschild-Simpson-Visser-type wormhole,
$ds^2=-\Big(1-\frac{2\,M}{\sqrt{x^2+b^2}}\Big)\,dt^2+\Big(1-\frac{2\,M}{\sqrt{x^2+b^2}}\Big)^{-1}\,\Big(\frac{dx^2}{\alpha^2}\Big)+(x^2+a^2)\,(d\theta^2+\sin^2
\theta\,d\phi^2)$. This wormhole is uniquely defined by a pair of key
parameters (length scales $a$ and $b$), together with the global monopole
charge $\alpha$. A noteworthy outcome of our investigation is the observation
that the energy-momentum tensor associated with this wormhole complies with
both the weak energy condition (WEC) and the null energy condition (NEC).
Furthermore, incorporation of global monopole charge introduces a substantial
influence on the curvature properties of wormhole space-time and various
associated physical quantities derived from this geometry.
