The galaxy presents as an elliptical morphology, displaying a smooth, centralized concentration of light. The luminous core transitions gradually outward, exhibiting a fading intensity towards its periphery. The overall color profile suggests a relatively evolved stellar population, with a yellowish-orange hue dominating the visual spectrum. The shape is elongated, with an approximate ratio of minor to major axis close to 0.65. There is no discernible spiral arm structure or prominent dust lanes visible, further supporting an elliptical classification. The galaxy lacks evidence of significant recent star formation activity, reinforcing its likely classification as an early-type galaxy.