The galaxy presents as a relatively smooth, elliptical structure. The core exhibits a reddish-orange hue, suggesting a population of older stars. Surrounding the core, there is a broader, somewhat fainter greenish-yellow halo. This halo implies a mix of stellar populations with potentially some ongoing star formation activity. The galaxy appears to be in a relaxed state, showing no obvious signs of recent major mergers or significant tidal disturbances. The shape is elongated, but not extremely so, leaning towards an intermediate ellipticity. Overall, the galaxy appears to be a massive system, but not exceptionally star forming.
