The galaxy presents a smooth, elliptical morphology. Its structure is dominated by a spheroidal component with a high degree of central concentration. There is no visible spiral structure, nor are there any apparent dust lanes. The galaxy exhibits a moderate ellipticity. Its color profile displays a redder central region, transitioning to bluer hues in the outer regions of the galactic halo, suggesting older stellar populations are centrally concentrated, while younger stars exist in the halo. There may be some evidence of minor tidal disturbances in the form of faint plumes, however its not significant. The galaxy appears relatively undisturbed, showing minimal signs of recent major merger activity.
