The galaxy presents a largely elliptical morphology, appearing quite smooth in structure. The central bulge is prominent and appears to be composed of older stellar populations, as suggested by its yellowish hue. This central region exhibits the highest luminosity. There's a gradual decrease in luminosity and intensity from the core outward.

The outer regions of the galaxy are less distinct, exhibiting a more diffuse and faint glow. No clear spiral arms or significant dust lanes are visible in the image. The overall roundness suggests the galaxy is viewed relatively face-on. There is no obvious signs of tidal disturbances or ongoing major mergers.
