The galaxy presents as a largely featureless elliptical with a smooth, concentrated light profile. The central region is bright and yellowish-white, suggestive of an older stellar population. The outer regions gradually fade into a diffuse halo, exhibiting a slightly redder hue compared to the core. The overall shape is nearly circular, showing minimal signs of disk-like structure or ongoing mergers. There is no indication of spiral arms or significant dust lanes. Given the smooth morphology, it's probable that star formation activity within the galaxy is suppressed, and its specific star formation rate is likely very low. There are no noticeable tidal features.
