The galaxy presents as a smooth, elliptical form. The light profile appears highly concentrated toward the center, suggesting a significant bulge component. There is a noticeable color gradient, with the core exhibiting a yellow-orange hue, indicative of an older stellar population. Moving outwards, the color shifts slightly towards redder tones, though the overall color remains consistent. The isophotes appear relatively circular, showing only a slight ellipticity. There are no clear indications of spiral arm structure, dust lanes, or recent star formation activity within the galaxy, implying it is likely an early-type galaxy. The apparent lack of features, combined with the high central concentration and color profile, points towards a well-evolved system.
