The galaxy presents a largely smooth and rounded morphology. A concentrated central bulge exhibits a warmer, yellowish-orange hue, which fades into a cooler, greenish halo. The galaxy shows no immediately apparent signs of spiral arm structure or significant tidal disturbances. It exhibits a relatively high degree of symmetry, with a smooth decline in luminosity outwards from the core, suggesting a lack of ongoing major merger activity. There may be slight disturbances but they are not easily apparent in the image. The overall light profile is dominated by the bulge component.
