The galaxy presents an elliptical morphology, appearing largely smooth and featureless. The light distribution suggests a centrally concentrated spheroid, with a gradual decrease in intensity outward. The core exhibits a yellowish-orange hue, potentially indicating an older stellar population with a lower rate of star formation. There are very faint indications of what might be a disk present, which could make this an S0 galaxy. The galaxy appears relatively isolated with no clear signs of major mergers or significant tidal disturbances. The galaxy is fairly round.
