The galaxy presents as a centrally concentrated, relatively smooth structure with a high degree of circularity. The core exhibits a luminous, yellowish-white hue, which likely indicates an older stellar population. Moving outwards, the galaxy's color transitions subtly toward a bluer shade, suggesting the presence of some younger stars in the outer regions. There are no discernible spiral arms or bar structures, and no clear signs of major ongoing mergers or tidal disturbances are evident from this image. The overall appearance implies a galaxy that is relatively evolved.
