Here's a finder chart and information about this event:
[link to www.skyandtelescope.com]
As of this morning it was about magnitude 4.6 or so, and still climbing in brightness!
[link to www.aavso.org]
It is evidently a classical nova of the Fe II spectral type, which is typically slower to evolve than the He/N type, and it is common in stars belonging to the galactic bulge.
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