The galaxy presents a generally smooth morphology, exhibiting characteristics consistent with an elliptical or lenticular type. The light distribution indicates a centrally concentrated bulge, with a gradual decrease in intensity towards the outer regions. There is little evidence of well-defined spiral arms or significant dust lanes. The galaxy exhibits a moderate elliptical shape with relatively even edges, with most of the light appearing to be concentrated in the central region. The core region displays a slightly yellowish color, transitioning to green hues in the outer regions, potentially indicative of varying stellar populations or dust content. Overall, the galaxy appears relatively undisturbed, with only subtle irregularities in its overall shape and brightness distribution. The galaxy is estimated to have a significant stellar mass and lies at a considerable redshift. The star formation rate is low, suggesting that it is a relatively quiescent system.
