  We have provided here a new class of interior solutions for anisotropic stars
admitting conformal motion in higher dimensional noncommutative spacetime. The
Einstein fields equations are solved by choosing a particular density
distribution function of Lorentzian type \cite{Nozari} under noncommutative
geometry. Several cases with dimensions $4D$ and higher, e.g. $5D$, $6D$ and
$11D$ have been discussed separately. An overall observation is that the model
parameters, such as density, radial pressure, transverse pressure, anisotropy
all are well behaved and represent a compact star with radius $4.17$ km.
However, emphasis has been given on the acceptability of the model from
physical point of view. As a consequence it is observed that higher dimensions,
i.e. beyond $4D$ spacetime, exhibit several interesting yet bizarre features
which are not at all untenable for a compact stellar model of strange quark
type and thus dictates a possibility of its extra dimensional existence.
