If anyone's interested, there have been a couple intriguing papers on arXiv over the last 2-3 days on SN2023ixf (
1,
2, and some others). It looks like the progenitor may have had an initial mass of ~11 solar masses, a little bit lower than initial estimates. But it's holding steady in brightness in optical/UV, so if you have access to even a small telescope, you might be able to see it.