The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth, diffused appearance. The core exhibits a bright, yellowish-white hue that gradually fades into a more diffuse, reddish halo. There is no apparent spiral arm structure or distinct dust lane features visible at this resolution. The galaxy appears relatively undisturbed, showing no major signs of ongoing merger activity or tidal distortions. The galaxy is quite compact with a relatively high surface brightness in the central region, suggesting a concentration of older stellar populations.
