This galaxy presents as a relatively smooth, centrally concentrated system. It exhibits a generally elliptical morphology with a high degree of circularity. The central region displays a bright, yellowish hue, suggesting an older stellar population. Moving outward from the core, the color gradually transitions to a more subdued and slightly bluer tone, potentially indicating the presence of younger stars in the outer regions, although this is less pronounced. There's no obvious spiral structure or significant dust lanes visible in the image. The overall impression is that of a mature galaxy, possibly undergoing relatively little active star formation at the present epoch.
