The galaxy presents as a somewhat elliptical structure with a smooth, concentrated central bulge exhibiting a yellowish hue, suggesting a population of older stars. A fainter, bluish-white disk surrounds the central bulge, indicative of some ongoing star formation. The overall morphology suggests a galaxy that is transitioning from a spiral-dominated structure to a more elliptical form. There is a slight hint of asymmetry in the outer regions, potentially suggesting a minor interaction or merger event in the past, though the main structure remains largely undisturbed.
