The galaxy presents a smooth, elliptical morphology, displaying a concentrated central bulge that diminishes gradually outwards. Its overall color appears to be yellowish-orange, indicating a population of older stars with lower star formation rates. There is no apparent spiral structure or dust lanes. It exhibits a fairly regular shape, without any major disturbances indicative of ongoing mergers. There may be some minor asymmetry present, but it is not severe. The isophotes appear smooth and well-blended, suggesting a fairly relaxed dynamical state.
