  Extended teleparallel gravity, characterized by $F(Q)$ function where $Q$ is
the non-metricity scalar, is one of the most promising approaches to general
relativity. In this paper, we reexamine a specific dynamical dark energy model,
which is indistinguishable from the $\Lambda$CDM model at present time and
exhibits a special event in the future, within $F(Q)$ gravity. To constrain the
free parameters of the model, we perform a Markov Chain Monte Carlo (MCMC)
analysis, using the last data from Pantheon$^{+}$ and the latest measurements
of the H(z) parameter combined. On the basis of this analysis, we have find
that our dynamical dark energy model, in the context of F(Q) gravity, lies in
the quintessence regime rather than in the phantom regime as in the case of
general relativity. Furthermore, this behaviour affects the future expansion of
the Universe as it becomes decelerating at $1\sigma$ confidence level for
$z<-0.5$ and showing a bounce at $z_{\text{B}}\approx -0.835$. Finally, we have
support our conclusion with a cosmographic analysis.
