The galaxy presents as a relatively smooth, elliptical-like object with a concentrated central bulge. The core appears bright and yellowish-white in color, possibly indicating an older stellar population. Moving outwards from the core, there is a diffuse, bluish halo, which may suggest the presence of a younger population of stars or some ongoing star formation. Overall, the galaxy appears fairly regular in shape, with no obvious signs of major disturbances or ongoing mergers, though there may be minor irregularities present. The light distribution suggests that it is mostly a spheroidal system.
