The galaxy presents a largely smooth morphology, with a high degree of central concentration. It appears generally round with a hint of possible disk structure. The galaxy exhibits a subtle color gradient, transitioning from a bluer central region to slightly redder outskirts. The overall shape is suggestive of an elliptical galaxy, though the aforementioned disk-like structure warrants further investigation. There appears to be a possible minor tidal disturbance or interaction with a smaller galaxy, but this is not definitive from the image alone. Star formation is present, but it is not widespread, and mostly confined to the galactic center. The galaxy shows no obvious signs of a recent major merger. The luminosity of the galaxy is relatively high, indicating a significant stellar population.
