The galaxy presents as a luminous, elliptical system with a smooth, concentrated light profile indicative of an early-type morphology. The core exhibits a bright, yellowish hue, likely representing an older stellar population. The surrounding halo displays a more diffuse, fainter light with subtle blueish tones, potentially suggestive of a small degree of recent star formation activity, though its contribution appears minor compared to the dominant older population. The overall shape is moderately elongated but largely featureless. There is no indication of a strong spiral structure or significant morphological disturbances from the image. The galaxy appears relatively isolated, without obvious signs of ongoing or recent mergers.
