The galaxy appears as a smooth, centrally concentrated object, roughly elliptical in shape. The core exhibits a bright, yellowish-orange color, suggesting a population of older stars and potentially a significant amount of dust obscuring bluer light. The galaxy's light profile decreases smoothly from the core outwards with no immediately obvious spiral arm structure or strong bar features. The outer regions appear fainter and redder, possibly indicating a lower density of younger stars or a more dust-rich environment in the outskirts. There is a subtle hint of a very faint, diffuse halo extending beyond the main body of the galaxy. No signs of major mergers or significant tidal disturbances are detected. The galaxy appears relatively undisturbed and quiescent.
