The galaxy presents a smooth, elliptical morphology. The light is concentrated toward the center with a gradual decrease in intensity towards the outer regions. The galaxy exhibits a noticeable, slightly elongated shape. No distinct spiral arm structures or prominent dust lanes are visible. A central bulge region is apparent as the brightest, most concentrated area of the galaxy. The overall color appears relatively uniform across the galaxy, suggesting a population of older stars with minimal recent star formation. There's no evidence of major ongoing merger activity, however some minor disturbance or interaction cannot be ruled out.
