The galaxy presents a generally smooth, elliptical morphology. A central bulge region is discernible, appearing as a bright, concentrated area, transitioning outward into a less luminous halo. The galaxy's color is somewhat uniform, displaying a redder hue characteristic of older stellar populations. There is very little evidence of spiral arms, star forming regions, or dust lanes. The shape is close to circular, with a slight elongation. There are no obvious signs of ongoing merger activity, or any major disturbances to the galaxy's structure.
