The galaxy presents as a primarily smooth, elliptical-like structure, exhibiting a high degree of central concentration. The light profile appears largely uniform and the overall form is generally rounded. The color index suggests a higher concentration of older stellar populations, with the galaxy appearing redder in overall color. There is no strong evidence of spiral arm structures or significant dust lanes. The galaxy displays a slight asymmetry, but no obvious signs of a major merger or tidal disturbances are visible. The morphology leans towards a relatively undisturbed system with a lack of pronounced features.
