The galaxy presents a relatively smooth, elliptical morphology. The central region exhibits a bright, concentrated core, suggesting a high stellar density. A gradual decrease in luminosity is observed moving outward from the core, forming a diffuse halo. There is a slight ellipticity to the overall shape, not perfectly circular, trending towards an oval. No prominent spiral arm structures or dust lanes are visible within the resolution of the image. The color profile indicates a redder hue, possibly indicating an older stellar population and lower star formation rate. There appears to be no significant interaction or major disturbance evident in its structure. A minor tidal feature is neither apparently present in the system, nor is a companion merger obvious, which contributes to the categorization as a smooth elliptical galaxy.
