Just had a quick look using the Lowell 53cm photometric telescope in its photometer previewer eyepiece. I couldn't see anything definite within the galaxy besides the conspicuous stellar (Seyfert) nucleus. My limit was fairly bright, Tsvetkov's star 9 (V=14.7) on the south-southeast side of the galaxy being a threshold object. So within the galaxy the limit would certainly be brighter, and I think quite a bit brighter than the reported magnitude. Awaiting CCD confirmation.... \Brian