  We combine deep imaging data from the CEERS early release JWST survey and HST
imaging from CANDELS to examine the size-mass relation of star-forming galaxies
and the morphology-quenching relation at stellar masses $\textrm{M}_{\star}
\geq 10^{9.5} \ \textrm{M}_{\odot}$ over the redshift range $0.5 < z < 5.5$. In
this study with a sample of 2,450 galaxies, we separate star-forming and
quiescent galaxies based on their star-formation activity and confirm that
star-forming and quiescent galaxies have different morphologies out to $z=5.5$,
extending the results of earlier studies out to higher redshifts. We find that
star-forming and quiescent galaxies have typical S\'{e}rsic indices of
$n\sim1.3$ and $n\sim4.3$, respectively. Focusing on star-forming galaxies, we
find that the slope of the size-mass relation is nearly constant with redshift,
as was found previously, but shows a modest increase at $z \sim 4.2$. The
intercept in the size-mass relation declines out to $z=5.5$ at rates that are
similar to what earlier studies found. The intrinsic scatter in the size-mass
relation is relatively constant out to $z=5.5$.
