The galaxy presents as a singular, relatively smooth structure. It exhibits a largely elliptical morphology, displaying a high degree of circularity. A slight deviation from perfect sphericity may be present, tending towards a more oblate shape. The galaxy appears to be largely undisturbed, showing no evidence of major mergers or significant tidal interactions. There are hints of subtle color gradients, trending from a redder core to slightly bluer outer regions. The overall color profile suggests a moderate amount of ongoing star formation activity, although older stellar populations likely dominate the mass budget.
