  We analyze pre-explosion ultraviolet (UV) imaging of the nearby Type II
supernova SN 2023ixf in search of precursor variability. No outbursts are seen
in observations obtained 15-20 yr prior to explosion to a limit of $L_{NUV}
\approx 1000~L_{sun}$ and $L_{NUV} \approx 2000~L_{sun}$. The time period of
these non-detections roughly corresponds to changes in the circumstellar
density inferred from early spectra and photometry.
