The galaxy presents as a relatively smooth, elliptical structure. Its central region exhibits a concentrated, bright core, suggesting a high density of stars. The color gradient transitions from a yellowish core to a slightly bluer halo, potentially indicating younger stellar populations in the outer regions, though this difference is subtle. The shape is generally ellipsoidal, with a slight elongation, but it doesn't appear highly flattened. There are no readily apparent spiral arms or major dust lanes visible, supporting a classification as an elliptical galaxy. There's no strong evidence of ongoing major merger activity; however, subtle disturbances in the outer regions cannot be ruled out without further investigation.
