The galaxy presents as a centrally concentrated, elliptical-like system. The core exhibits a bright, yellowish-orange hue, indicative of an older stellar population. The light smoothly diffuses outward from the nucleus. The overall structure appears relatively smooth, with no prominent spiral arms or distinct dust lanes visible. Faint asymmetric features are detected on the right side of the galaxy, which may be minor tidal disturbances or hints of an ongoing merger.
