The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that dominates the overall light profile. The core displays a warmer color, shifting towards redder wavelengths, potentially indicating an older stellar population in the galaxy's nucleus. Moving outwards from the center, the light profile gradually diffuses into a more indistinct halo, displaying tinges of green and blue. This indicates that the halo is bluer than the bulge but also has a combination of more than one color. The overall symmetry suggests a relatively undisturbed morphology, with little evidence of strong tidal interactions or major mergers. Faint outer regions hint at a substantial spatial extent.
