This galaxy presents as a moderately luminous object with an elliptical morphology. The light profile appears relatively smooth, suggesting a spheroid-dominated structure. There is a possible disturbance in the light distribution, though it is subtle. The galaxy exhibits a color gradient, transitioning from a yellow-orange hue in the central regions to a slightly bluer periphery. This color variation may indicate differences in stellar populations or dust content across the galaxy. The redshift suggests it is a relatively distant object. Overall, the galaxy appears to be a fairly massive, evolved system, with a potentially subdued level of star formation. There are indications of a past interaction or minor merger event that could have influenced its morphology.
