Hey Maurits,
Personally I see it as a very, very niche item overall. It's just a classic pair of absorption lines at 589.0nm and 589.6nm. You can identify flare eruption kernals, if you study that sort of thing, but really won't be doing it unless you have some active sunspots to do it with often likely. You might see some bit of flare coming through there though (but less profound compared to HA), when one occurs, but you need a lot more activity than what's going on now. Otherwise, it's just going to appear like the photosphere (well, lower chromosphere technically, but it will look like the photosphere for features). No obvious non-subtle features that will be different than will not be noted in another wavelength that shows the features of the photosphere. Frankly, g-band is going to offer more contrast on convection cells and calcium k will show a lot more different features from the photosphere, especially faculae areas will be immediately different and obvious compared to sodium or even continuum. So it's a personal thing really. Personally I think CaK, HA and any short (395~430nm) or long wavelength (610~656nm) of your choice (seeing dependent) for the photosphere rounds out the kit with most non-subtle features able to be noted without requiring a huge aperture & excellent seeing to be able to experience.
I certainly would not bother with it for just a general "photosphere" or white light narrowband filter. I would only consider it again if you're specifically trying to see or capture things that are highlighted by the wavelength in high resolution (flare kernals).
It is certainly nice to have options though!
Very best,