The galaxy presents as a moderately luminous elliptical system at an approximate distance, indicated by its redshift. Morphologically, it exhibits a generally smooth, spheroidal structure with a high degree of central concentration. The main body of the galaxy appears relatively featureless, lacking prominent spiral arms or distinct dust lanes.

There is a color gradient visible, with a bluer hue towards the central region that shifts toward redder colors in the outer portions of the galaxy. This suggests ongoing or recent star formation towards the center, and an older stellar population on the outskirts. The redder colors in the outer regions indicate a greater proportion of older, cooler stars, while the bluer colors in the inner regions suggest a younger, hotter stellar population and possibly some level of current star formation.

There is only a slight indication of a disk-like structure.
