The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. Surrounding the core, a diffuse blue halo extends outwards, potentially indicating ongoing, albeit low, star formation activity or the presence of a population of younger, bluer stars. There's no discernible spiral structure or prominent dust lanes visible in the image. The overall appearance suggests a mature galaxy, likely an elliptical or lenticular type, without any signs of major ongoing mergers or significant tidal disturbances.
