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This paper constructs two immediate extensions of the existing anisotropicsolutions in the context of Einstein-Maxwell framework by employing minimalgeometric deformation. To achieve this, we assume a static spherical interiorinitially filled with anisotropic fluid and call it a seed source. We extendthis matter configuration by including a new source whose impact on theself-gravitating system is governed by a decoupling parameter. The chargedfield equations analogous to the total fluid source are formulated. We thenimplement a transformation on the radial metric potential that divides thefield equations into two new under-determined systems, corresponding to theinitial and new sources. The first of them is addressed by taking twowell-known metric ansatz so that the number of unknowns can be tackled.Further, the vanishing of total anisotropy and complexity-free constraints areused to solve the second set. The estimated radius and mass of a compact star$4U~1820-30$ is utilized to interpret the resulting solutions graphically fordifferent values of the charge and decoupling parameter $\omega$. We concludethat our both developed models are physically acceptable for all parametricvalues except $\omega=1$.

Effects of Charge and Gravitational Decoupling on Complexity and Isotropization of Anisotropic Models