The galaxy presents as a relatively smooth, elliptical morphology, although there is a hint of a disk-like structure present. Its shape is predominantly round, with a slight elongation evident. The galaxy exhibits a strong central bulge, which appears bright and yellowish, suggesting a high concentration of older stellar populations. The outer regions are fainter and display a bluer hue, potentially indicative of more recent star formation. There is no visible evidence of major ongoing merging activity, though a minor disturbance can't be fully ruled out based on the subtle structural asymmetries. Overall, the galaxy appears to be an intermediate to high-mass system, with a moderate amount of star formation.
