The galaxy presents as a centrally concentrated, smooth system, consistent with an early-type morphology. The core exhibits a bright, yellowish hue, which gradually fades into a more diffuse, red-tinged halo. There is no apparent spiral structure or distinct dust lanes. The overall impression is of an elliptical galaxy with a relatively passive stellar population. There may be some minor morphological disturbances present in the halo indicating a possible merger event in the past.
