Hi Glen,
Nope, haven't seen it and I think it is unlikely that any of us will see the actual nebula given the emission lines it shines at.
This is not a classical PNe like the ones formed at the end of the lives of sun-like low to medium mass stars, but a ring-type wind-blown shell nebula formed from a LBV star.
There is a very detailed paper (using the echellle spectrograph on the AAT) on the properties of this star and the nebula surrounding it here:
http://cdsads.u-strasbg.fr/full/1994A%26A...281..833S
And the writers conclude that the central star should be re-classified as a W11 wolf-rayet star and that it possesses some properties in common with the nearby AG Carinae (which also has a dusty ring).
While the star (at ~mag 11 is certainly observable, the nebula is not really visible (at visual wavelengths). It is a very, very young nebula being only 2x10^4 yrs old
Best,
Les D
Contributing Editor
AS&T