The galaxy presents as a relatively smooth, elliptical-like structure. The core exhibits a bright, concentrated luminosity, suggesting a high stellar density and/or possible active galactic nucleus. There is a gradual decrease in surface brightness extending outwards from the core. The overall color appears to be slightly yellowish, which could indicate an older stellar population. The galaxy shows no apparent signs of significant disturbances or major mergers; the morphology appears largely undisturbed. There is no obvious disk structure or spiral arm features. The shape is close to circular.
