The galaxy presents an elliptical morphology, appearing relatively smooth in structure. There is a noticeable color gradient, transitioning from a yellower central bulge to slightly bluer hues in the outer regions of the disk. The galaxy is moderately inclined with respect to our line of sight, showing a flattened, elongated appearance. There is no strong evidence of prominent spiral arms or a well-defined disk structure. The galaxy exhibits a moderate amount of light and seems to be a relatively large galaxy. The redder areas of the galaxy appear as bright concentrated regions suggesting older stellar populations, while the bluer regions may indicate ongoing or recent star formation.
