This galaxy presents a largely smooth and centrally concentrated appearance. The core exhibits a bright, yellowish-white hue, indicative of an older stellar population. Surrounding the core is a more diffuse, bluish halo. The blue color suggests the presence of younger, hotter stars, implying ongoing or recent star formation, albeit at a moderate level. 

The overall shape appears somewhat elliptical, verging on circular, with only a slight deviation from perfect roundness. There's no discernible evidence of spiral arms or a distinct disk structure, and no obvious signs of tidal disturbances or merging activity are present. The morphology suggests this galaxy is a relatively evolved system, possibly an elliptical or lenticular type.
