The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, with a bright, yellow-tinted core that gradually fades into the surrounding galactic halo. There appears to be little to no discernible structure such as spiral arms or a prominent disk. There's a subtle color gradient, transitioning from yellower hues at the core to redder tones in the outer regions, suggesting possible variations in stellar populations or dust content. No signs of any major mergers are visible, although the possibility of minor disturbances cannot be ruled out given the image's resolution.
