The galaxy exhibits a generally smooth morphology, with a round shape. The central region displays a bright, concentrated luminosity, transitioning into a more diffuse halo. There's a subtle color gradient, with the central core appearing more yellowish-white, suggesting an older stellar population, while the outer regions have a more reddish hue, potentially indicating some lower levels of recent star formation or dust extinction. The structure appears largely undisturbed, lacking any obvious signs of a major merger event. Faint extensions may be visible, potentially indicative of tidal interactions or minor disturbances.
