The galaxy presents as a largely smooth, centrally concentrated object, elliptical in appearance with a noticeable yellow-red color gradient toward the core. The profile suggests a relatively high degree of sphericity; the galaxy exhibits only a slight deviation from a perfectly circular shape. There are subtle hints of faint features or disturbances, though no clear tidal tails or signs of recent major mergers are apparent. Its color profile suggests an older stellar population with less ongoing star formation. The system appears to be relatively isolated. 
