I've come across a similar discussion on what the star type is - the stumbling block is whether the picture in the Codex was enhanced. They never did come to a conclusion
Even if it's enhanced and even if you take that picture as evidence, this is a cold M or K at most, likely a giant and you still need the whole 9-body subsystem to be very close to see anything of the sort in the picture. It could also be T Tauri (one of those that look basically like M and you want to scoop but can't), but then this needs to be even closer. Or S class, but those are few and far in between and people generally visit them. The distance requirement to get this shot is the biggest problem with that picture.
And there literally aren't really supergiants anywhere remotely close enough for this to work, and with those you're looking at this station orbiting a lava world, possibly. Funnily enough, I've been to two out of four in a reasonable, and one is Beetlejuice, but the other was some HIP system that wasn't actually all that scanned, but it also didn't have anything interesting. The supergiants are close-ish, but you're already looking at >1k LY trips if I recall correctly so I'd not really count them as primary candidates.
There is another option that this is a shot of a secondary star in a system, not a primary one. This reduces the distance requirements, and primary could be far away.
So, you could be looking at some system where the primary is some O, B, A, or F, with a secondary of maybe T and a gas giant paired in a close-ish orbit, far away, and the shot is of the T star, and you don't actually see the gas giant in the picture.
A spansh query for something like this, with distance from the entrance >100kLS gives me 12 candidates.
www.spansh.co.uk
And we have 38 Aquarii:
www.spansh.co.uk
which is the only one that has a gas giant with 8 moons, but the gas giant is around the main star, not the one far out.