The galaxy presents a generally smooth and elliptical morphology. It appears concentrated, with a bright central region that gradually diffuses outward. There is a subtle color gradient, with the central region appearing slightly bluer compared to the outer edges which exhibit a redder hue. No distinct spiral arms or significant dust lanes are discernible within the galaxy’s structure. There is some indication of minor distortions or faint tidal features that hint at past or ongoing interactions with other galaxies, but no actively merging galaxies are obvious in the image.
