The galaxy presents as a largely featureless, smooth elliptical. It exhibits a concentrated, bright core with a fairly rapid decline in luminosity moving outwards. The overall shape is nearly circular, showing minimal elongation or distortion, indicative of a relaxed system. There are no discernible spiral arms, dust lanes, or other prominent features. The galaxy displays a smooth color gradient, transitioning from a yellowish-white core to a bluer halo, potentially indicating a difference in stellar populations, where the core is populated with older, redder stars, and the halo contains younger, bluer stars. There are no visible signs of any major recent or ongoing merger events. The galaxy appears isolated, suggesting a gravitationally stable system.
