This galaxy presents a largely smooth morphology, appearing elliptical in shape, with a high degree of roundness. The central region exhibits a brighter, more concentrated luminosity profile, suggesting a prominent galactic nucleus. There's a noticeable color gradient, with the core appearing more yellow-white, potentially indicating an older stellar population dominating this region. The outer regions fade gradually into the background, displaying a slightly bluer hue, which might indicate the presence of younger stars, though to a smaller degree. There is no evidence of spiral arms or a defined disk structure visible in the image. No signs of active galactic nuclei features are present. There are no obvious signs of recent major merger events or significant tidal disturbances within the galaxy's structure.
