The galaxy presents as a relatively smooth, featureless elliptical or lenticular galaxy. It appears elongated, with an intermediate roundness, not quite spherical but also not a highly flattened disk. The light distribution suggests a concentrated central bulge. There is a yellow-orange hue, with a smooth gradient, which could indicate an older stellar population dominating the light emitted, with little ongoing star formation. There is a slight hint of blue at the galaxy edges. No distinct spiral arms or significant dust lanes are visible. There is no obvious evidence of a major merger, or significant tidal disturbances.
