The galaxy presents a somewhat elliptical morphology, appearing elongated rather than perfectly spherical. The light distribution suggests a prominent central bulge that is bright. The outer regions fade in brightness, indicating lower stellar density or light intensity at the edges. 

Hints of what could be spiral arms or dust lanes are present, although the resolution limits a conclusive determination. The color profile indicates a relatively old stellar population, with a yellowish or reddish hue dominating the central region. Bluer tones are sparsely scattered, which may suggest ongoing, but low, levels of star formation within the galaxy. The overall structure suggests a galaxy undergoing transformation, potentially settling into a more passive state.
