https://www.nasa.gov/image-feature/goddard/2018/hubbles-lonely-firework-display
Roughly 50 million light-years away lies a somewhat overlooked little galaxy named NGC 1559. Pictured here by Hubble’s Wide Field Camera 3,
this barred spiral lies in the little-observed southern constellation of Reticulum (the Reticule).
NGC 1559 has massive spiral arms chock-full of star formation, and is receding from us at a speed of about 808 miles per second (1,300 kilometers per second).
The galaxy contains the mass of around ten billion suns — while this may sound like a lot, it is over 20 times less massive than the Milky Way. Although NGC 1559
appears in the sky near one of our closest galaxy neighbors, the Large Magellanic Cloud (LMC), this is just a trick of perspective. In reality, NGC 1559 is
physically nowhere near the LMC in space — in fact, it truly is a loner, lacking the company of any nearby galaxies or membership of any galaxy cluster.