  This paper investigates the geometry of compact stellar objects via Noether
symmetry strategy in the framework of curvature-matter coupled gravity. For
this purpose, we assume the specific model of this theory to evaluate Noether
equations, symmetry generators and corresponding conserved parameters. We use
conserved parameters to examine some fascinating attributes of the compact
objects for suitable values of the model parameters. It is analyzed that
compact objects in this theory depend on the conserved quantities and model
parameters. We find that the obtained solutions provide the viability of this
process as they are compatible with the astrophysical data.
