The galaxy presents as an elliptical or lenticular galaxy. It exhibits a largely smooth morphology with minimal visual evidence of spiral arms or significant dust lanes. The galaxy is approximately round in shape. There are no prominent tidal features or indications of a recent major merger event, though subtle asymmetries or minor disturbances cannot be ruled out based on this image alone. The galaxy's core appears relatively bright, with the overall light profile gradually decreasing towards the outer edges. Color gradients across the galaxy are subtle. The central region appears slightly redder compared to the outer regions, which seem bluer. This could indicate differences in stellar populations, with older, redder stars concentrated in the center and younger, bluer stars being more dispersed.
