M110



M110 (also known as Messier 110, 'The Edward Young Star' and NGC 205) is a dwarf elliptical galaxy that is a satellite of the Andromeda Galaxy. It is at a distance of 824.76 ± 27.59 kpc from Terra.

M110 contains some dust and hints of recent star formation, which is unusual for dwarf elliptical galaxies in general. Unlike M32, M110 does not show evidence for a supermassive black hole at its center.

There are no known Ancient Gates, Golden Bazaars, or planned expeditions to this galaxy.

