  We report the discovery of J0624-6948, a low-surface brightness radio ring,
lying between the Galactic Plane and the Large Magellanic Cloud (LMC). It was
first detected at 888 MHz with the Australian Square Kilometre Array Pathfinder
(ASKAP), and with a diameter of ~196 arcsec. This source has phenomenological
similarities to Odd Radio Circles (ORCs). Significant differences to the known
ORCs - a flatter radio spectral index, the lack of a prominent central galaxy
as a possible host, and larger apparent size - suggest that J0624-6948 may be a
different type of object. We argue that the most plausible explanation for
J0624-6948 is an intergalactic supernova remnant due to a star that resided in
the LMC outskirts that had undergone a single-degenerate type Ia supernova, and
we are seeing its remnant expand into a rarefied, intergalactic environment. We
also examine if a massive star or a white dwarf binary ejected from either
galaxy could be the supernova progenitor. Finally, we consider several other
hypotheses for the nature of the object, including the jets of an active
galactic nucleus (AGN) or the remnant of a nearby stellar super-flare.

High Energy Astrophysical Phenomena;Cosmology and Nongalactic Astrophysics