  In this paper, we consider isotropic solution and extend it to two different
exact well-behaved spherical anisotropic solutions through minimal geometric
deformation method in $f(R,T,R_{\rho\eta}T^{\rho\eta})$ gravity. We only deform
the radial metric component that separates the field equations into two sets
corresponding to their original sources. The first set corresponds to perfect
matter distribution while the other set exhibits the effects of additional
source, i.e., anisotropy. The isotropic system is resolved by assuming the
metric potentials proposed by Krori-Barua while the second set needs one
constraint to be solved. The physical acceptability and consistency of the
obtained solutions are analyzed through graphical analysis of effective matter
components and energy bounds. We also examine mass, surface redshift and
compactness of the resulting solutions. For particular values of the decoupling
parameter, our both solutions turn out to be viable and stable. We conclude
that this curvature-matter coupling gravity provides more stable solutions
corresponding to a self-gravitating geometry.
