The galaxy presents a generally smooth and elliptical morphology. It appears largely spheroidal with high degree of central concentration of light. The core region exhibits a yellowish hue, suggesting a population of older stars, possibly dominated by red giants and low-mass stars. There is a notable absence of clearly defined spiral arms or prominent dust lanes, supporting its classification as an elliptical galaxy. The isophotes appear relatively regular and undisturbed. While there is some color variation, it doesn't point to ongoing, widespread star formation within the galaxy body. The light profile indicates a relatively high mass. Its red-shifted nature places it at a considerable distance. No signs of a major ongoing merger are apparent in its structure. There might be some minor asymmetry, potentially indicating the presence of an ongoing disturbance.
