The galaxy appears to be a relatively smooth, elliptical galaxy. The central region presents a concentrated luminosity profile, indicative of a significant bulge component. There is a gradual falloff in surface brightness from the core outwards, with no distinct spiral arm structures visible. The galaxy's shape is generally elongated, with a ratio of minor to major axes suggesting an E4-E5 morphological type. Faint blue tinges are visible in the outer regions which may indicate a small amount of on-going star formation. No significant signs of tidal disturbances or ongoing mergers are immediately apparent. The overall color is consistent with a population of older stars, though some subtle color gradients suggest variations in stellar populations or dust content within the galaxy.
