The galaxy presents as an elongated, elliptical structure. Its central region exhibits a bright, concentrated luminosity, suggesting a high density of stellar populations. The light profile appears smooth, with a gradual decrease in brightness moving outward from the core. There is a slight asymmetry in the outer isophotes, hinting at a minor disturbance or interaction. Overall, the galaxy lacks prominent features such as spiral arms or dust lanes, indicating that it is likely a mature system with a well-mixed stellar population. A reddish hue can be seen on the periphery, particularly at the extreme ends of the elongation. There is no evidence of a strong tidal distortion, nor does it appear to be actively merging.
