  We analyze the recent astrophysical constraints in the context of a hadronic
equation of state (EoS), in which the baryonic matter is subject to chiral
symmetry restoration. We show that with such EoS it is possible to reconcile
the modern constraints on the neutron star (NS) mass, radius, and tidal
deformability (TD). We find that the softening of the EoS, required by the TD
constraint of a canonical $1.4~M_\odot$ NS, followed by a subsequent
stiffening, required by the $2~M_\odot$ constraint, is driven by the appearance
of $\Delta$ matter due to partial restoration of chiral symmetry. Consequently,
a purely hadronic EoS that accounts for the fundamental properties of quantum
chromodynamics linked to the dynamical emergence of parity doubling with
degenerate masses of nucleons and $\Delta$ resonances can be fully consistent
with multi-messenger data. Therefore, with the present constraints on the EoS,
the conclusion about the existence of the quark matter in the stellar core may
still be premature.
