The ultra-compact dwarf galaxy, dubbed M60-UCD1, was found in what's known as the Virgo cluster of galaxies, researchers said.
Imagine the distance between the Sun and the star nearest to it - Alpha Centauri. That's a distance of about 4 light years. Now, imagine as many as 10,000 of our Suns crammed into that relatively small space.
That is about the density of a galaxy discovered by an international team of astronomers led by a Michigan State University faculty member.
The galaxy was discovered in the Virgo cluster of galaxies, a collection of galaxies located about 54 million light years from our own Milky Way.
What makes M60-UCD1, so remarkable is that about half of its mass is found within a radius of only about 80 light years. This would make the density of stars about 15,000 times greater than found in Earth's neighbourhood in the Milky Way.
The discovery of ultra-compact galaxies is relatively new - only within the past 10 years or so. Until then, astronomers could see these "things" way off in the distance but assumed they were either single stars or very-distant galaxies.
Another intriguing aspect of this galaxy is the presence of a bright X-ray source in its centre. One explanation for this is a giant black hole weighing in at some 10 million times the mass of our Sun.
The possible massive black hole, combined with the high galaxy mass and Sun-like levels of elements found in the stars, favour the latter idea.
A giant black hole at the centre of M60-UCD1 helps tip the scales against the scenario where this galaxy was once a star cluster, since such large black holes are not found in these types of objects.
The galaxy was discovered using NASA's Hubble Space Telescope. Follow-up observations were done with NASA's Chandra X-ray Observatory and ground-based optical telescopes, including the Keck 10-metre telescope in Hawaii.
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