The galaxy presents as a centrally concentrated object with a generally smooth morphology. The core region exhibits a yellowish-white hue, suggestive of an older stellar population. Surrounding the core is a more diffuse halo of bluish light, implying the presence of younger, hotter stars and potential ongoing star formation, albeit at a low rate. The galaxy appears largely undisturbed with no obvious signs of recent mergers or tidal interactions. There may be a slight, very subtle, elongation to the galactic structure, but overall it presents as largely elliptical.
