The galaxy presents as a relatively smooth and rounded object. It exhibits a concentrated central region, possibly a bulge, with a yellowish hue indicating older stellar populations and a lack of ongoing, intense star formation. The outer regions transition to a bluer color, suggesting the presence of younger stars, though not in significant quantities. There is no clear disk structure visible, and no signs of recent major merger events. The overall structure is largely undisturbed and elliptical in nature, appearing symmetrical.
