The galaxy presents a largely smooth, elliptical morphology, with a high degree of central concentration. The core is bright and appears relatively featureless. A slight extension of the galaxy is visible in the surrounding envelope. There is subtle color variation, trending toward slightly bluer hues at the outskirts as compared to the core. There is no evident spiral structure or distinct dust lanes. The galaxy seems to have only minor distortions, not demonstrating a strong merging signature.
