The galaxy presents a generally smooth, elliptical morphology. The core exhibits a concentrated, bright, yellowish-white luminosity, suggestive of an older stellar population. There is a subtle, but evident, color gradient extending outward from the core. The outer regions display a diffuse, reddish hue, indicating a broader distribution of evolved stars and potentially some dust obscuration. The overall structure appears largely undisturbed, with no obvious signs of tidal features or major interactions. There may be a faint, subtle, and partial ring structure surrounding the core.
