Triangulum galaxy
This galaxy has an inclination of 54° to the line of sight from the Earth, allowing the structure to be examined without significant obstruction by gas and dust. The disk of the Triangulum Galaxy appears warped out to a radius of about 8 kpc. There may be a halo surrounding the galaxy, but there is no bulge at the center. This is an isolated galaxy and there are no indications of recent interactions with other galaxies, and it lacks the small following galaxies or tidal tails associated with the Milky Way.