The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a high degree of luminosity, appearing nearly uniform in color and texture. Moving outward from the core, the light gradually diminishes, forming a relatively diffused halo. A subtle color gradient can be observed, transitioning from yellowish-white at the center to slightly redder hues in the outer regions. There is a notable absence of distinct spiral arms or well-defined dust lanes. The galaxy appears largely undisturbed, lacking significant signs of tidal interactions or ongoing major mergers, although slight asymmetries in the outer halo cannot be ruled out. Overall, this galaxy exhibits characteristics consistent with a passively evolving system.
