The galaxy exhibits a flattened, elliptical morphology. It displays a notable central bulge with a high degree of concentration of light intensity. The bulge appears nearly spherical, grading into a disk-like structure with a high degree of inclination. The visible color gradient suggests older stellar populations concentrated in the bulge, and the subtle bluish tones at the edges might indicate ongoing or recent star formation in the outer regions. There is no apparent spiral structure or distinct dust lanes observed. The overall color profile is dominated by redder wavelengths, indicating a relatively evolved stellar population and limited recent star formation. The isophotes are relatively smooth and symmetrical.
