The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a high concentration of luminosity, appearing bright and yellowish-orange in color. This suggests an older stellar population dominating the core. The galaxy's light gradually diminishes outwards from the center, transitioning to a slightly greener hue. There is a very slight elongation observed, but overall it appears quite regular in shape. No distinct spiral arms or dust lanes are apparent. A faint halo may exist, but it is poorly defined against the background sky. There are no obvious signs of recent major merger activity or significant tidal disturbances.
