This galaxy presents as an edge-on spiral. There is a prominent central bulge that appears to be quite luminous and smoothly distributed. The disk is very thin and elongated, with a bright, nearly homogenous appearance of the disk with no noticeable spiral arm structure discernible. There are hints of dust lane absorption along the midplane of the disk, but they appear quite faint. The galaxy shows no obvious signs of major mergers or significant tidal disturbances. The galaxy's overall color appears relatively red, suggesting an older stellar population and possibly lower star formation activity. The rounded shape of the bulge further reinforces the idea that this is an older galaxy.
