The galaxy appears to be a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, displaying a high degree of circularity. The core region presents a bright, yellowish-white hue, suggesting a dominant population of older stars. The outer regions appear fainter and have a slightly bluer tint compared to the core, hinting at the presence of younger stars or ongoing, albeit weak, star formation. There is no visually discernible evidence of spiral arms, bars, or any major morphological disturbances indicative of recent mergers. The galaxy is well-defined and doesn't exhibit a fuzzy, irregular appearance, indicating a stable and relaxed structure.
