  The impact of nuclear structure has garnered considerable attention in the
high-energy nuclear physics community in recent years. This work focuses on
studying the potential nuclear cluster structure in $^{16}\text{O}$ nuclei
using anisotropic flow observables in $\rm O+O$ collisions at 200 GeV.
Employing an improved AMPT model with various cluster structure configurations,
we find that an extended effective parton formation time is necessary to align
with the recent STAR experimental data. In addition, we reveal that the
presented flow observables serve as sensitive probes for differentiating
configurations of $\alpha$-clustering of $^{16}\text{O}$ nuclei. The systematic
AMPT calculations presented in this paper, along with comprehensive comparisons
to forthcoming experimental measurements at RHIC and the LHC, pave the way for
a novel approach to investigate the $\alpha$-clustering structure of
$^{16}\text{O}$ nuclei using $\rm O+O$ collisions at the ultra-relativistic
energies.
