The galaxy appears as a small, faint spiral, viewed edge-on. It has a clearly defined disk, marked by a dark dust lane running along its mid-plane, bisecting the galaxy. Faint spiral arm structures extend outwards from the central bulge, which is compact and bright. There might be a slight warping of the disk. The overall color suggests a population of older stars in the bulge and possibly younger stars concentrated in the disk. There is potential evidence of minor disturbances and a potential merger event occurring. 
