  While rotation-supported gas disks are known to exist as early as at z~7, it
is still a general belief that stellar disks form late in the Universe. This
picture is now being challenged by the observations from the James Webb Space
Telescope (JWST), which have revealed a large number of disk-like galaxies that
could be at z>3, with some being candidates at z>7. As an early formation of
stellar disks will greatly impact our theory of galaxy formation and evolution,
it is important to determine when such systems first emerged. To date, there is
only one confirmed case at z>5 ("Twister-z5") reported in the literature. Here
we present D-CEERS-z5289, a stellar disk at $z=5.289\pm0.001$ discovered using
the archival JWST NIRCam imaging and NIRSpec spectroscopic data. This galaxy
has a highly regular edge-on disk morphology, extends to ~6.2 kpc along its
major axis, and has an effective radius of ~1.3--1.4 kpc. By analyzing its
10-band spectral energy distribution using four different tools, we find that
it has a high stellar mass of 10^{9.5-10.0} Msun. Its age is in the range of
330--510 Myr, and it has a mild star formation rate of 10--30 Msun/yr. It is
conceivable that this galaxy assembled its stellar mass by secular growth.
Unfortunately, the current spectroscopic data do not allow the derivation of
its rotation curve. Nevertheless, the width of its H$\alpha$ line (~345 km/s)
from the partial slit coverage on one side of the disk suggests that it could
be a fast-rotating system.
