The galaxy presents as a single, relatively smooth, elliptical-shaped object. The core exhibits a concentrated, bright region, suggesting a significant density of stars in the galactic nucleus. A gradual decrease in luminosity extends outward from the center, with no distinct features such as spiral arms or bars visible. The galaxy appears generally round in shape, with minor irregularities present. The overall color profile suggests a population of older stars, as indicated by the reddish hue. There is no prominent evidence of ongoing major star formation. Faint tidal features are not observed, which points towards the absence of recent major merger events. Minor disturbances are also absent.
