  This paper constructs two immediate extensions of the existing anisotropic
solutions in the context of Einstein-Maxwell framework by employing minimal
geometric deformation. To achieve this, we assume a static spherical interior
initially filled with anisotropic fluid and call it a seed source. We extend
this matter configuration by including a new source whose impact on the
self-gravitating system is governed by a decoupling parameter. The charged
field equations analogous to the total fluid source are formulated. We then
implement a transformation on the radial metric potential that divides the
field equations into two new under-determined systems, corresponding to the
initial and new sources. The first of them is addressed by taking two
well-known metric ansatz so that the number of unknowns can be tackled.
Further, the vanishing of total anisotropy and complexity-free constraints are
used 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 for
different values of the charge and decoupling parameter $\omega$. We conclude
that our both developed models are physically acceptable for all parametric
values except $\omega=1$.
