The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears predominantly elliptical or lenticular. The core exhibits a yellowish-white color, suggesting an older stellar population dominating the central region. A fainter, bluish halo surrounds the core, which may indicate the presence of younger stars or a more diffuse distribution of stars compared to the central region.

The overall shape is largely rounded, with no obvious signs of strong tidal interactions or major disturbances. There is a hint of asymmetry, but not to a degree that suggests a recent major merger. Minor disturbances cannot be ruled out from visual inspection alone. 

The galaxy is moderately bright, exhibiting a consistent but not intense luminosity profile from the center outwards. The colors indicate ongoing, albeit low, star formation. The overall appearance is consistent with a galaxy that has largely ceased active star formation, retaining a smoother morphology.
