The galaxy presents a largely smooth, elliptical morphology. It exhibits a pronounced central bulge that appears slightly elongated. A faint disk structure may be present, hinted at by a subtle flattening and some irregularity in the outer regions, though this is not sharply defined. The galaxy's color profile suggests a predominantly older stellar population, indicated by the yellowish-orange hue, particularly concentrated in the bulge. There is evidence of some bluer regions, especially on one side of the galaxy, suggesting regions of potential ongoing or recent star formation. No significant signs of tidal disturbances or major merger events are apparent, though some minor asymmetry is noted in its structure.
