The galaxy presents a primarily smooth morphology. The light distribution suggests a centrally concentrated spheroid, indicative of an elliptical galaxy or the bulge component of a spiral. There is a subtle elongation, with the overall shape being close to round but trending towards a more elliptical form. No distinct spiral arm structures or significant dust lanes are visible. The color profile suggests a dominance of older stellar populations, as the galaxy appears somewhat redder in the outer regions and slightly bluer towards the center, possibly indicating some ongoing or recent star formation in the core. No signs of major mergers or tidal disturbances are apparent, though subtle asymmetry could point to minor past interactions.