The galaxy presents as a largely smooth, centrally concentrated object. It exhibits an elliptical morphology, appearing mostly rounded with a slight elongation. A dominant, bright central bulge is observed, transitioning to a less luminous halo. The color profile suggests an older stellar population, based on the redder hues, particularly towards the center. There is faint evidence of star formation activity, particularly at the edges, indicated by some blue coloring at the edges. No apparent signs of major mergers or significant tidal disturbances are visible. The galaxy does appear smooth and undisturbed, consistent with an evolved system.
