The galaxy presents as a relatively smooth, elliptical structure with a high degree of central concentration. Its color index suggests a population of older stars, with a slightly redder hue dominating the overall appearance. The galaxy exhibits a near-circular morphology. There are no obvious signs of active star formation regions, tidal tails, or significant dust lanes discernible in this image, suggesting a quiescent state. Any faint, disturbed features are potentially indicative of minor gravitational interactions, but the overall morphology remains largely undisturbed, supporting the smooth classification.
