This galaxy presents an elongated, elliptical morphology. The central region exhibits a bright, concentrated core, possibly indicating a significant concentration of older stellar populations. Moving outwards from the center, the galaxy displays a smoother, more diffuse light distribution.  The overall color suggests a population of older stars, with a hint of blue possibly indicating some ongoing, though limited, star formation. There are no obvious signs of spiral arm structure or significant dust lanes visible in this image. The galaxy appears relatively undisturbed, with no clear signs of recent major mergers or interactions. It is primarily smooth in appearance.
