The galaxy appears as a singular, centrally concentrated object with a smooth, relatively featureless morphology. It displays a slightly elongated, but generally rounded shape, and is a relatively small galaxy. The color appears to be primarily a pale blue-white, suggesting a population of hot, young stars, and a small amount of on-going star formation. There is no obvious visual indication of a spiral structure, bar, or tidal disturbances indicative of recent major mergers. There is also no central bulge. The galaxy seems to be isolated.
