Abstract
Galaxy formation models predict that galaxies grow inside-out, becoming larger over time. While observations broadly support this paradigm, the nature and timescales of this growth remain poorly constrained. We report the discovery of an extremely faint and young (∼600 Myr) stellar component in the outer regions of the nearby galaxy Messier 74 (M74). Using deep optical imaging from the TST telescope at the Teide Observatory, reaching surface brightness limits of ∼30-31.5 mag arcsec
−2
in the
g, r
, and
i
bands, we detect stellar emission extending well beyond the previously known disc radius of ∼14 kpc. This newly identified component reaches galactocentric distances of ∼30 kpc, effectively doubling the known size of the stellar disc and matching the extent of the H
I
disc. The revised size of M74 places it in the upper envelope of the mass–size relations. The young age of the outer stellar population suggests a recent episode of disc growth, potentially occurring on timescales shorter than ∼1 Gyr. We discuss a possible scenario in which a past flyby interaction with UGC 1176 may have triggered this extended star formation. Further studies of galaxies with similarly deep imaging will be key to determining whether such rapid outer disc growth is common or exceptional.