Quote Originally Posted by Uwe Glahn View Post
I remember a lecture of Bernd Gährken about CS in PN for small aperture. Funny, but this CS is one of the few which is visible in binoculars
That's the point and this is actually the main difficulty in observing this PN under less than optimal conditions: Separating it from the glow of the CS (not the true progenitor star, which is now a White Dwarf, but its bright G5 companion).