The galaxy appears to be a relatively smooth, disk-like structure, although not perfectly symmetrical. It exhibits a central bulge with a more concentrated luminosity. Faint spiral arm-like features may exist but are not well-defined. The disk component is seen at an oblique angle. The color is largely uniform across the galaxy, with a slight bluer tint. It may be a galaxy with ongoing, though not exceptionally high, levels of star formation. No strong signs of tidal disturbances or major mergers are readily apparent. 
