The galaxy presents as a single, largely featureless spheroid. There is a concentration of light towards the galactic center, appearing reddish, possibly indicating an older stellar population and/or significant dust obscuration in the core. Moving outwards from the center, the color shifts towards a bluer hue. The blue color could potentially indicate a younger stellar population in the outer regions or simply less dust in the outer regions.

The galaxy exhibits a smooth profile with no obvious spiral arm structure or prominent dust lanes. The overall shape is nearly circular, with minimal ellipticity observed. There are no apparent signs of major tidal disturbances or ongoing mergers, although there are faint hints of some minor disturbances to the galaxy's smooth profile.
