The galaxy appears as a relatively smooth, elliptical-shaped object with a bright central core. There's a subtle color gradient observed, transitioning from a yellowish-white center to a faint bluish halo at the edges. No distinct spiral arms or bar structures are discernible. The overall morphology suggests an early-type galaxy, possibly an elliptical or lenticular. There is no obvious ongoing major merger event, although a minor asymmetry or disturbance cannot be completely ruled out given the image quality. The central concentration of light indicates a possible bulge component. The colors suggest a population of older stars are dominating the light output.
