  In this work, we investigate whether the compact object at the center of the
Milky Way is a naked singularity described by the $\textit{q}$-metric
spacetime. Our fitting of the astrometric and spectroscopic data for the S2
star implies that similarly to the Schwarzschild black hole, the
$\textit{q}$-metric naked singularity offers a satisfactory fit to the observed
measurements. Additionally, it is shown that the shadow produced by the naked
singularity is consistent with the shadow observed by the Event Horizon
Telescope collaboration for Sgr-A*. It is worth mentioning that the spatial
distribution of the S-stars favors the notion that the compact object at the
center of our Galaxy can be described by an almost static spacetime. Based on
these findings, the $\textit{q}$-metric naked singularity turns up as a
compelling candidate for further investigation.
