The galaxy presents as a relatively smooth, elliptical structure. A concentrated central bulge of older stars appears to be the dominant feature, emitting primarily in the redder wavelengths, suggesting an older stellar population. This central region is surrounded by a more diffuse halo with a bluer hue, potentially indicating ongoing, albeit subdued, star formation within the galactic disk. The overall shape is moderately elongated, not perfectly spherical, but not highly elongated either. There is no obvious evidence of major disturbances, such as tidal tails or asymmetrical structures suggesting recent or ongoing major mergers. Minor irregularities, such as subtle asymmetries in the outer halo, could indicate minor interactions or internal processes at play.
