The galaxy presents a largely smooth, elliptical morphology. It appears primarily as a spheroid of light, with the highest intensity concentrated in the core region. A subtle color gradient is observable from the center outwards. The core shows a more whitish hue, grading into a faint blue tint in the surrounding regions, hinting at older stellar populations in the core. There is little evidence of spiral arms or a distinct disk. The overall structure suggests a fairly relaxed system, potentially consistent with an early-type galaxy that has undergone significant dynamical evolution. Slight, almost imperceptible, disturbances may be present within the light distribution, potentially suggestive of a minor ongoing interaction. However, the dominant visual impression is one of a smooth and relatively undisturbed system.
