The galaxy presents as a centrally concentrated, generally smooth structure. The core exhibits a bright, yellowish-white hue, potentially indicating an older stellar population. A diffuse, bluish halo extends outward from the central region, suggesting the presence of some younger, hotter stars. There is a lack of prominent spiral arms or a distinct disk-like structure, and it appears mostly round in shape. The morphology suggests an early-type galaxy, possibly an elliptical, with a relatively high degree of central concentration. There might be subtle disturbances in the outer halo, but overall, the galaxy doesn't show evidence of major mergers or strong tidal interactions.
