The galaxy presents as a relatively smooth, elliptical morphology. There is a discernible central bulge, exhibiting a yellowish-orange hue, potentially indicative of an older stellar population. The outer regions fade into a less defined halo, appearing slightly bluer than the core. There are no prominent spiral arms or dust lanes visible in this image. The overall shape is generally round, with only a slight elongation. There's no obvious evidence of any major interactions or mergers. The galaxy seems to be relatively quiescent, not showing significant features associated with rapid star formation.
