The galaxy presents as a relatively smooth, elliptical structure. There is a central concentration of light, appearing yellowish-orange, which likely indicates an older stellar population dominating the core region. Surrounding this core, a bluer halo is visible, possibly suggestive of more recent or ongoing star formation in the outer regions, but the fraction is low. The overall shape appears fairly round with only slight ellipticity. No prominent spiral arms or bars are discernible. The galaxy appears relatively isolated, with no obvious signs of major tidal disturbances or ongoing mergers, although minor disturbance cannot be ruled out.
