  In this article we study the structure and stability of compact astrophysical
objects which are ruled by the dark energy equation of state (EoS). The
existence of dark energy is important for explaining the current accelerated
expansion of the universe. Exact solutions to Einstein field equations (EFE)
have been found by considering particularized metric potential, Finch and Skea
ansatz \cite{Finch}. The obtained solutions are relevant to the explanation of
compact fluid sphere. Further, we have observed at the junction interface, the
interior solution is matched with the Schwarzschild's exterior vacuum solution.
Based on that, we have noticed the obtained solutions are well in agreement
with the observed maximum mass bound of $\approx$ 2$M_{\bigodot}$, namely, PSR
J1416-2230, Vela X-1, 4U 1608-52, Her X-1 and PSR J1903+327, whose predictable
masses and radii are not compatible with the standard neutron star models.
Also, the stability of the stellar configuration has been discussed briefly, by
considering the energy conditions, surface redshift, compactness, mass-radius
relation in terms of the state parameter ($\omega$). Finally, we demonstrate
that the features so obtained are physically acceptable and consistent with the
observed/reported data \citep{Gondek-Rosinska,Glendenning}. Thus, the present
dark energy equation of state appears talented regarding the presence of
several exotic astrophysical matters.
