The galaxy presents a largely smooth, elliptical morphology. The color profile indicates a significant presence of older stellar populations, with a yellowish-orange hue dominating the central region. This central region exhibits a high degree of concentration, suggesting a substantial bulge component. Fainter, less concentrated light extends outwards from the core, with a gradual falloff in brightness. While the overall appearance is smooth, there is a subtle hint of a disk-like structure. No apparent signs of tidal disturbances or ongoing major mergers are evident.
