The galaxy presents as a relatively smooth, elliptical-like structure with a high degree of central concentration. There is a distinct, bright central bulge that appears largely spheroidal and emits primarily yellow and white light, suggesting a population of older stars. The outer regions appear fainter and bluer, with a less-defined edge, potentially indicating a more extended distribution of younger stars or ongoing star formation. The shape is somewhat elongated, deviating slightly from a perfect sphere but without any obvious signs of a prominent disk or spiral arms. There are no visible signs of major mergers or tidal disturbances, although a very subtle asymmetry may be present in the outer halo.
