The galaxy appears to be a relatively smooth, elliptical system with a concentrated central bulge. The overall color profile suggests a population of older stars, as indicated by the yellow-red hue of the bulge, although there is a subtle greenish tint in the outer regions. There are no obvious spiral arms or dust lanes visible. The galaxy's light profile fades gradually from the center outward, suggesting a diffuse stellar halo. There is a slight elongation to the galaxy's shape, but overall it appears largely spheroidal. There is some indication of minor tidal disturbances, hinting at potential past interactions with smaller galaxies.
