  In this paper, we investigate topologically charged Morris-Thorne-type
wormholes using various shape function forms. We solve the Einstein field
equations incorporating an anisotropic energy-momentum tensor and obtain
different physical quantities associated with the matter content. A crucial
aspect of this study is the non-exotic matter distribution, examined through
the evaluation of energy conditions, and exploring how different shape
functions impact these conditions. Additionally, the anisotropy parameter is
calculated to quantify the extent of attractive or repulsive behavior. Our
study demonstrates that for different types of shape function forms, the energy
conditions are influenced by the global monopole parameter. Our findings
provide valuable insights for further theoretical explorations of these
fascinating hypothetical structures in the realm of general relativity and
beyond
