The Dorado Group is a loose concentration of galaxies containing both spirals and ellipticals. It is generally considered a 'galaxy group' but may approach the size of a 'galaxy cluster'. It lies primarily in the southern constellation Dorado and is one of the richest galaxy groups of the Southern Hemisphere. Gérard de Vaucouleurs was the first to identify it in 1975 as a large complex nebulae II in the Dorado region, designating it as G16.
NGC 1566, one of the brightest members of the Dorado Group (Spitzer Space Telescope image)
Peculiar galaxy NGC 1487 is located about 30 million light-years away in the constellation of Eridanus.
Dorado is a constellation in the Southern Sky. It was named in the late 16th century and is now one of the 88 modern constellations. Its name refers to the mahi-mahi, which is known as dorado ("golden") in Spanish, although it has also been depicted as a swordfish. Dorado contains most of the Large Magellanic Cloud, the remainder being in the constellation Mensa. The South Ecliptic pole also lies within this constellation.
The constellation Dorado as it can be seen by the naked eye
NGC 1566 is an intermediate spiral galaxy.
LEDA 89996 is a classic example of a spiral galaxy.