The galaxy presents as a largely featureless, elliptical or spheroidal structure. It exhibits a smooth, centrally concentrated light distribution with a gradual decline in luminosity moving outward from the core. The color profile suggests an older stellar population, with a yellowish-orange hue dominating the central region. There is a subtle color gradient, with the outer regions appearing slightly bluer, which could indicate more recent, albeit limited, star formation activity in these areas, or simply a difference in the metallicity of the stars. The galaxy appears relatively isolated, without any obvious signs of recent major merger events or strong tidal interactions. The morphology is consistent with a high degree of rotational symmetry.
