The galaxy presents as an elliptical morphology, appearing largely smooth and spheroidally shaped. Its color is predominantly yellow-orange, with a higher concentration of this hue towards the center suggesting an older stellar population in the galactic nucleus. Peripheral to the core, some subtle blue-green tinges are observed, potentially indicating regions of more recent, though subdued, star formation activity. There is no clear evidence of spiral arm structures or significant dust lanes, and the overall appearance suggests a relaxed system with minimal tidal disruption. The galaxy exhibits a high degree of central concentration and roundedness. There is no apparent merger activity.
