@cosmos4u Not easily, as it looks like most of the brightness is in the diffuse outer coma, which is still largely hidden by the sky. In photometry, I can detect faint signal in the g' stack out to ~1' from the nucleus (i.e., ~2' diameter), within which I get g' ~ 10.3 (V ~ 10.1 at solar color, which is not quite right but maybe close). However, CCOR-1 images showed a coma twice this diameter, with a ~0.4 mag difference between the two apertures. That yields an extremely rough V ~ 9.7, from this pile of assumptions. Could be a few 0.1 mag brighter, since g' is actually more sensitive to the gas than CCOR-1, and the gas is more diffuse than the dust (leading to a bigger difference between the apertures).