The galaxy presents as a centrally concentrated system with a smooth, elliptical morphology. The core exhibits a bright, relatively uniform luminosity profile, suggesting an older stellar population. Moving outwards, the galaxy displays a gradual decrease in surface brightness. The color gradient transitions from a yellowish-white core to a bluer halo, hinting at a possible shift in stellar populations from older, redder stars in the center to younger, bluer stars in the outer regions. There is no clear evidence of spiral arms or prominent dust lanes. The galaxy shows a high degree of rotational symmetry, appearing mostly circular. There are no obvious signs of tidal distortions or ongoing merger activity.
