Lenticular galaxy
NGC 4526. Its dark lanes of dust and bright diffuse glow make the galaxy appear to hang like a halo in the emptiness of space.
This galaxy is known to have a colossal supermassive black hole at its center that has the mass of 450 million Suns.
Galaxy
NGC 1291. Though the galaxy is quite old, ~ 12 billion years, it is marked by an unusual ring where newborn stars are igniting.
NGC 1291 is located ~ 33 million ly away in the constellation Eridanus. It is what's known as a barred galaxy, because its central region is dominated by a long bar of stars (the bar is within the blue circle and looks like the letter "S"). The stars that appear blue in the central, bulge region of the galaxy are older; most of the gas there was previously used up by earlier generations of stars. When galaxies are young and gas-rich, stellar bars drive gas toward the center, feeding star formation.
Over time, as the fuel runs out, the central regions become quiescent and star-formation activity shifts to the outskirts of a galaxy. There, spiral density waves and resonances induced by the central bar help convert gas to stars. The outer ring, seen here in red, is one such resonance area, where gas has been trapped and ignited into star-forming frenzy.