The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge, characterized by a yellow-orange hue indicative of an older stellar population. The light distribution gradually diminishes from the core, lacking prominent spiral arm structures or distinct features. There is a faint greenish-blue halo surrounding the central region, possibly indicative of some ongoing, albeit subdued, star formation activity. The galaxy appears relatively undisturbed, showing no signs of major mergers or significant tidal interactions.
