The galaxy presents a predominantly smooth, elliptical morphology. The core exhibits a high surface brightness with a yellowish hue, suggesting an older stellar population. Moving outwards from the core, a diffuse halo is observed, fading into the background sky. A subtle, disk-like structure is barely discernible, with faint arms or features hinting at a possible spiral or lenticular morphology, though the smoothness of the light distribution dominates. There is no apparent evidence of recent or ongoing major merger events, and the galaxy appears relatively undisturbed. The overall color suggests a lower rate of star formation.
