The galaxy presents as a relatively smooth, elliptical morphology. Its color profile suggests an aging stellar population, with a concentration of older, redder stars towards the galactic center, as indicated by the yellow-orange hue of the core. The outer regions show hints of blue, potentially suggesting the presence of younger, hotter stars or perhaps some ongoing, albeit minimal, star formation. The overall shape is not perfectly spherical, exhibiting a slight elongation, reminiscent of an E3-E5 elliptical classification. There is no obvious evidence of spiral arms, bar structures, or significant dust lanes within the visible light spectrum. No significant tidal disturbances or merger remnants are immediately apparent, suggesting a relatively isolated evolutionary path, though subtle asymmetries could potentially indicate past interactions. 
