The galaxy presents a smooth, elliptical morphology. The light is concentrated towards the center, with a gradual decrease in intensity outwards. The shape is slightly elongated, with an apparent axis ratio of approximately 0.9, indicating a moderate flattening. There is little to no discernible structure such as spiral arms or dust lanes. The galaxy exhibits a color gradient, appearing yellower in the core region and transitioning to slightly bluer hues in the outer regions. This suggests an older stellar population concentrated in the center, with potentially younger stars distributed in the outer regions.
