NGC 2275 is classified as a flocculent (or fluffy-looking) spiral galaxy. It’s about 67 million light-years away in the direction of the constellation Cancer. It’s fluffy spiral arms are the result of a slowdown in star formation, and virtually no new stars are being formed in center of the galaxy which is unusually large and relatively empty. Essentially all its gas was converted into stars long ago.
Image Credit: NASA / ESA