The galaxy presents as a relatively smooth, elliptical object. The central bulge exhibits a pronounced reddish hue, suggesting an older stellar population. Surrounding the bulge is a diffuse, greenish-yellow halo. This halo may indicate the presence of a younger stellar population or ongoing, though perhaps weak, star formation. The overall shape is somewhat rounded, with only minor deviations from a perfect elliptical form. There's no clear evidence of strong tidal disturbances or interactions with other galaxies, indicating it has likely evolved relatively undisturbed. No distinct spiral arm structures are apparent; the galaxy appears to be a fairly mature system with a dominant spheroidal component.
