Comparison of GRB host galaxy absolute magnitudes (or upper limits) from the SHOALS sample at 3.6 microns (Perley et al. 2016), and from various HST observations at 1.1-1.6 microns (Tanvir et al. 2012; McGuire et al. 2016; Lyman et al. 2017); note that these are in a fixed observed band, and so substantially different rest-frame band at different redshifts. Under the assumption that the host of GRB 250314A dominates the emission in the F150W2 band, the observations are consistent with other GRB hosts at high-z.