The galaxy presents a largely smooth, elliptical morphology. Its core is a bright, concentrated region of light, surrounded by a more diffuse halo that gradually fades into the background. There is minimal evidence of spiral arms or prominent dust lanes. The galaxy appears relatively rounded in shape, with no significant elongation or distortion evident. Some subtle color variations are present within the galaxy, with a slightly bluer hue in the outer regions compared to the yellower core. This suggests the presence of younger stars in the outer regions. No significant tidal features or signs of ongoing major mergers are apparent, but subtle disturbances cannot be completely ruled out.