This galaxy presents as a relatively smooth, centrally concentrated object. The light distribution indicates a primarily elliptical morphology, with no obvious spiral arm structures or prominent dust lanes visible. The color profile suggests a population of older stars, indicated by the reddish-yellow hue, particularly in the central region. There is a slight color gradient from the core to the outer regions, with a subtle shift towards bluer colors in the periphery, possibly indicating some degree of ongoing star formation, though at a low rate. The overall appearance is of a mature, relatively undisturbed galaxy.
