The galaxy presents a generally smooth, elliptical morphology. Its color profile suggests a higher concentration of older stellar populations, with a prominent central bulge exhibiting a yellowish-white hue. A surrounding, diffuse halo appears slightly bluer, potentially indicating the presence of younger stars or a lower metallicity population in the outer regions, although this could also be a color effect. There is no apparent spiral arm structure or strong evidence of active star formation within the visible light spectrum. The galaxy shows a high degree of rotational symmetry, presenting with an axial ratio suggesting it is nearly circular, viewed close to face-on. There are no obvious signs of a major merger event or tidal disturbances. The galaxy exhibits low-level star formation overall.
