The galaxy presents as a centrally concentrated, relatively smooth object. The light distribution suggests a bulge-dominated morphology, with a bright, yellowish core that transitions to a fainter, bluer halo. The galaxy exhibits an elliptical-like shape; it appears almost round. There are no immediately obvious signs of spiral arms or a prominent disk structure. There are some subtle disturbances in the outer regions of the halo, hinting at possible minor interactions or internal asymmetries. Overall, the galaxy appears to be a fairly well-formed elliptical galaxy with a moderate amount of star formation.
