M33, a galaxy known for its high rate of star formation, is being observed by the Hubble Space Telescope.
Unlike other galaxies, M33's star formation is not fueled by galactic collision but rather by a large amount of dust, gas, and ionized hydrogen clouds.
Researchers have found evidence of high-mass star formation through collisions between massive molecular clouds within M33.
The Hubble image reveals reddish clouds of ionized hydrogen mixed with dark dust lanes, showcasing the abundance of stars in M33.