The galaxy presents as a relatively smooth, elliptical object. It exhibits a strong central concentration of light, with a yellowish hue, suggesting an older stellar population. The isophotes appear generally regular, with a slight elongation, indicating a moderate ellipticity. There is no discernible spiral arm structure or dust lane features visible. A subtle color gradient is observed, transitioning from the central yellow-dominant bulge to slightly bluer colors in the outer regions of the galaxy, which suggest a presence of younger stars in the outskirts. No tidal disturbances or signs of a major merger event are apparent. The galaxy appears largely undisturbed and evolved.
