  We report on new Very Long Baseline Interferometry radio measurements of
supernova 2014C in the spiral galaxy NGC 7331, made with the European VLBI
Network ~5 yr after the explosion, as well as on flux density measurements made
with the Jansky Very Large Array (VLA). SN 2014C was an unusual supernova,
initially of Type Ib, but over the course of ~1 yr it developed strong
H$\alpha$ lines, implying the onset of strong interaction with some H-rich
circumstellar medium (CSM). The expanding shock-front interacted with a dense
shell of circumstellar material during the first year, but has now emerged from
the dense shell and is expanding into the lower density CSM beyond. Our new
VLBI observations show a relatively clear shell structure and continued
expansion with some deceleration, with a suggestion that the deceleration is
increasing at the latest times. Our multi-frequency VLA observations show a
relatively flat powerlaw spectrum with $S_\nu \propto \nu^{-0.56 \pm 0.03}$,
and show no decline in the radio luminosity since $t\sim1$ yr.
