The galaxy presents a largely smooth, elliptical morphology. It appears concentrated, with a bright central bulge that fades gradually into a diffuse halo. There is a subtle elongation, suggesting a shape that deviates slightly from a perfect circle. The color profile indicates an older stellar population, with a dominant yellowish hue in the core region. Some bluer tones can be observed in the outer regions, suggesting the possibility of ongoing, though subdued, star formation. No prominent spiral arms or dust lanes are visible. There is no clear evidence of any major tidal disturbances or ongoing mergers, though a slight asymmetry might indicate past interactions. The galaxy's overall structure suggests it is a relatively evolved system, possibly undergoing a quiescent phase of star formation.
