Unfortunately we have only H, H, H and H of
the Balmer series. H is a broad line, about 6000 kms-1
wide at the continuum level, H is 2400 kms-1 wide and
H 1100 kms-1 wide.
The H line is too near to the plate limit to be able to say
something meaningful. No line has an indication of a P Cyg structure.
The Paschen series is visible up to n=28, with a clear progression
from n=25 downwards. The emissions are sharp and narrow at our
resolution and show no trace of underlying absorption lines.