The galaxy presents a largely smooth and elliptical morphology. It exhibits a concentrated central bulge with a yellow-orange hue, indicative of an older stellar population. The light distribution suggests minimal dust lanes or spiral arm structures. The outer regions of the galaxy gradually fade into the background, with no apparent tidal features or strong gravitational interactions with nearby galaxies. The overall shape appears close to circular. The light is very concentrated in the center of the object.

Based on the galaxy's colors, it is likely that the star formation rate is low.
