The galaxy presents a largely smooth and elliptical morphology. It exhibits a concentrated, bright central bulge which gradually fades into a more diffuse halo. No distinct spiral arms or prominent dust lanes are discernible. The galaxy appears generally round in shape. There are no visible signs of any major ongoing merger activity or strong tidal distortions. The color profile suggests a relatively evolved stellar population, lacking significant blue light indicative of recent or current high levels of star formation.
