This galaxy exhibits a largely smooth morphology, with a dominant, somewhat circular central bulge. The overall color profile indicates a population of stars that spans a broad range of ages. The yellow-white core suggests a high concentration of older stars. Subtle green hues surrounding the core might point to the presence of some ongoing, albeit low-level, star formation. There is little evidence of spiral arm structure or significant dust lanes; the galaxy presents as an object with primarily elliptical characteristics. The light is concentrated towards the center, indicating a high degree of central mass concentration. There is no visible evidence to suggest a major ongoing merger event.
