  S$H_0$ES $VI$-band photometry for classical Cepheids in the keystone galaxy
NGC4258 yield discrepant absolute magnitudes. Specifically, the 2016 and 2022
published S$H_0$ES Cepheid data for NGC4258 exhibit a substantial offset of
$\Delta W_{0,VI}\simeq0^{\rm m}.3$. That adds to a suite of existing concerns
associated with the S$H_0$ES analysis, which in sum imply that their relatively
non-changing Hubble constant for nearly twenty years warrants scrutiny.
