The galaxy presents as an elliptical morphology, appearing largely spheroidal in shape with a high degree of central concentration. The light profile transitions smoothly from a bright, yellowish core to a more diffuse, reddish halo. There is little evidence of distinct spiral arms or a prominent disk structure, suggesting that it is likely an early-type galaxy. No obvious signs of recent or ongoing major mergers are observed; the morphology appears relatively undisturbed. The overall color gradient indicates that the core likely contains an older stellar population.
