The galaxy presents a largely smooth and elliptical morphology. The light distribution is concentrated towards the center, displaying a bright, unresolved core, indicative of a substantial spheroidal component. Moving outwards from the core, the light gradually diffuses, with a relatively smooth gradient and a subtle color change; the core exhibits a yellowish-white hue, shifting towards a somewhat bluer color in the outer regions. The isophotes appear to be moderately elliptical, and there is no obvious indication of spiral arms or a prominent disk structure. There are no notable signs of strong tidal interactions or major mergers, although a subtle asymmetry in the outer envelope cannot be entirely ruled out.
