The galaxy presents as a centrally concentrated elliptical type, exhibiting a smooth, largely featureless morphology. The core region displays a bright, yellowish-white hue, suggesting an older stellar population. There is a gradual radial falloff in surface brightness from the core outward. The isophotes appear generally regular, though with slight indications of elongation. No distinct spiral arms, dust lanes, or signs of recent major merger events are visible. Subtle color gradients suggest a potential variation in stellar populations with radius, possibly indicating past minor interactions or accretion events. The overall structure indicates a dynamically relaxed system, with ongoing or recently quenched star formation activity.
