The galaxy presents as an elliptical morphology, exhibiting a smooth, concentrated light profile with a high degree of central symmetry. Its overall shape appears nearly round, showing minimal deviation from circularity. There are no visible spiral arms or distinct disk features, suggesting a classification leaning towards an early-type galaxy. The color gradient indicates a predominantly older stellar population, with a reddish hue prominent in the core and diminishing towards the outer regions, which exhibit a slightly bluer color. There is no obvious indication of significant dust lanes or active star formation regions in the visual spectrum. The galaxy is relatively isolated, showing no strong signs of tidal interactions or ongoing mergers.
