The galaxy presents as a disk-shaped structure, viewed at a high inclination, close to edge-on. There is a prominent central bulge that appears relatively smooth. The disk shows evidence of structure, with some suggestion of clumpy regions. There appears to be some dust absorption along the midplane of the disk, obscuring the light from behind. There are indications of some tidal features or minor disturbances present. The galaxy appears to be undergoing relatively little star formation, with a mix of intermediate to old stellar populations. 
