The galaxy presents as a single, concentrated object with a smooth, elliptical morphology. A notable central bulge exhibits a yellowish-orange hue, suggesting a population of older, evolved stars. The outer regions of the galaxy fade into a less defined halo, appearing slightly bluer in color, potentially indicating some ongoing, albeit weak, star formation activity. There is no discernible disk structure, spiral arms, or significant dust lanes visible in this image. The galaxy appears relatively undisturbed, without obvious signs of tidal interactions or ongoing mergers. The overall morphology indicates a system that is likely dynamically relaxed.
