The galaxy presents a generally smooth, elliptical morphology. The light is centrally concentrated, with a diffuse and extended halo. The core exhibits a yellowish-white hue, suggestive of an older stellar population. There are no prominent spiral arm structures, bars, or obvious dust lanes visible. The overall roundness indicates a minimal degree of rotational support and a more pressure-supported system. No obvious signs of tidal disturbances or ongoing mergers are apparent; the galaxy appears relatively undisturbed. Based on the light profile, this is likely a massive galaxy with a low star formation rate.
