The galaxy presents as a relatively smooth, elliptical structure with a dominant central bulge. There is a subtle flattening, suggesting it is not perfectly spherical. The core exhibits a concentrated, bright, yellowish-white hue, indicating a significant population of older stars. Extending outward from the core, the color transitions to a more diffuse, yellow-orange gradient. There is a slight suggestion of a faint, extended disk component, although this feature is not clearly defined and appears mostly smooth and devoid of distinct spiral arms. A hint of greenish-blue tint is present within the galaxy's halo region, potentially indicative of younger stellar populations or low-level star formation activity. There is no evident presence of dust lanes, tidal tails, or other significant morphological disturbances, suggesting it is a relatively undisturbed system. Overall, the galaxy appears as a mature system with a largely passive stellar population.
