The galaxy appears to be an elliptical type, exhibiting a generally smooth and concentrated morphology. A bright, yellowish-white central region dominates the galaxy's structure, suggesting an older stellar population is heavily concentrated in the core. Moving outward from the center, the color gradually shifts towards a slightly redder hue, before blending with a cooler faint blue halo. There is no apparent spiral structure, or significant dust lanes visible. The galaxy exhibits a high degree of circular symmetry, showing a profile that is nearly round, with only the slightest elongation discernable. There are no obvious signs of tidal disturbances or ongoing mergers, suggesting the galaxy is relatively undisturbed. The extended halo fades gradually into the background. Overall, the galaxy presents a relaxed and well-defined structure characteristic of a mature elliptical galaxy.
