The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape appears elliptical or spheroidal, exhibiting a high degree of roundness with only minor deviations from perfect circular symmetry. There is a pronounced central bulge that is significantly brighter than the outer regions of the galaxy. There are no obvious signs of spiral arms, bar structures, or significant dust lanes within the visible light data. Subtle indications of minor disturbances or tidal features are present, possibly hinting at past or ongoing gravitational interactions with other galaxies. Given the color gradient, the galaxy is likely composed of an older stellar population, exhibiting limited current star formation. 
