  We present hydrodynamical star-forming simulations in the Milgromian dynamics
(MOND) framework of a gas-rich disc galaxy with properties similar to AGC
114905, which has recently been argued to have a rotation curve (RC) that is
inconsistent with the MOND prediction. Our first model considers the galaxy in
isolation, while our second model includes an external field of $0.05 \,
a_{_0}$, the estimated gravitational field from large-scale structure. We show
that isophotes in the face-on view can differ from circular at the 50% level.
This could mislead observers into overestimating the inclination $i$ between
disc and sky planes. Because RCs require a correction factor of $1/\sin i$, the
actual RC could be much higher than reported by observers. This plausibly
reconciles AGC 114905 with MOND expectations.
