  The Odd Radio Circles are newly identified diffuse radio sources at ~1 GHz
frequency, with edge-brightened nearly circular morphology, which is remarkably
similar to supernova remnants although a physical association with previous
population of Galactic supernova remnants is challenging due to detections of
the Odd Radio Circles at high Galactic latitudes. Here, a serendipitous
identification of a new source in a LOFAR 144 MHz image with similar morphology
as that of Odd Radio Circles is reported. This is the first reported
identification of an Odd Radio Circle at a very low frequency and with the
LOFAR.
