The galaxy appears to be a disk galaxy, oriented edge-on relative to our line of sight. It has a notable bulge, which is slightly brighter and more concentrated than the disk. There are possible dust lanes visible bisecting the galaxy, however, they're not easily distinguished. It shows very few if any signs of recent major disturbances or mergers and appears generally smooth. It's moderately luminous and relatively massive. It is likely not forming stars at a high rate, it shows a low specific star formation rate, and likely has an older stellar population. It is elongated in shape, but not extremely so.
