This galaxy appears to be a spiral galaxy with a moderate bulge. The spiral arms are somewhat tightly wound, with what seems to be a relatively bright galactic center. The galaxy is not perfectly face-on, but tilted at a small angle, but the spiral arm structure can still be seen. Some segments of the arms are brighter than others, which indicates ongoing or recent star formation activity. The bulge size is moderate and the galaxy does not appear to be undergoing any major merging events. The overall color of the galaxy indicates that the it is composed of old stellar populations. The color is slightly bluer in the spiral arms than the central bulge. From its moderate luminosity, it has a mass that is around the mass of the Milky Way.
