The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge with a gradual decrease in luminosity outward. The color profile suggests a relatively old stellar population, with a redder hue concentrated towards the core region and a slight bluer tint at the edges. No prominent spiral arm structures or dust lanes are discernible. The galaxy appears largely undisturbed, with no obvious signs of recent major merger events or tidal distortions. There may be minor disturbances in the surrounding area, however it is not clear if this impacts the core body. Overall, the galaxy appears as a well-defined, elliptical galaxy.
