  Anomalous Cepheids (ACs) are metal-deficient, core-helium-burning pulsating
stars with masses in the range 1.2-2.2 M_S. Until recently, all known ACs were
pure single-mode pulsators. The first candidate for an AC pulsating in more
than one radial mode - OGLE-GAL-ACEP-091 - was recently identified in the Milky
Way based on the photometric database of the Optical Gravitational Lensing
Experiment (OGLE) survey. We analyze this object showing that it is actually a
triple-mode pulsator. Its position in the Petersen diagram, the light-curve
morphology quantified by Fourier coefficients, and absolute magnitudes derived
from the Gaia parallax are consistent with the assumption that
OGLE-GAL-ACEP-091 is an AC. Our grid of linear pulsation models indicates that
OGLE-GAL-ACEP-091 is a 1.8 M_S star with a metallicity of about [Fe/H] = -0.5
dex.
