  In this paper, we develop two anisotropic solutions for static
self-gravitating spherical structure in the presence of electromagnetic field
through gravitational decoupling approach in $f(G,T)$ theory, where $G$ and $T$
denote the Gauss-Bonnet term and trace of the energy-momentum tensor,
respectively. The extra source with isotropic seed sector is responsible for
generating anisotropy in the spacetime. The system of field equations is
decoupled into two arrays by using minimal geometric deformation in the radial
component. The first set portrays the isotropic regime whereas the second set
represents the anisotropic system. The metric coefficients of the Krori-Barua
spacetime are employed to extract solution of the first set while two
constraints on the radial and temporal components of the extra source yield the
corresponding two solutions. Finally, we investigate the influence of charge
and decoupling parameter on the physical viability and stability of the
obtained solutions. We conclude that the resulting solutions in this modified
theory indicate more feasible and stable structures.
