The galaxy presents a largely smooth, elliptical morphology. Its color profile suggests an older stellar population, with a dominant yellowish-orange hue concentrated toward the core. There is subtle evidence of a very faint, diffuse, greenish outer halo. This feature may indicate areas of ongoing, low-level star formation, although the galaxy overall appears relatively quiescent. No distinct spiral arms or prominent dust lanes are visible. There are no strong indications of recent major merger events based on morphological disturbances; the overall structure is fairly regular and undisturbed. The galaxy exhibits a high degree of circularity in its shape, suggesting a spheroidal structure.
