The galaxy presents as a single, relatively smooth structure, exhibiting a centrally concentrated luminosity profile. The primary color is a yellowish-white, suggesting an older stellar population in the central bulge region. A bluer halo surrounds the central region, indicative of some ongoing, though not particularly vigorous, star formation. The galaxy shows a high degree of circularity, lacking any obvious signs of a spiral arm structure or a highly elongated shape. There are no clear indications of tidal tails, streams, or strong morphological disturbances typically associated with recent major merger events. The overall appearance is consistent with a relatively undisturbed, moderately massive system with a dominant spheroidal component.
