The galaxy presents as an elliptical structure, elongated along a major axis. The central region exhibits a higher surface brightness, appearing relatively smooth and featureless, indicative of an older stellar population. The color gradient shifts from a more yellowish hue in the core to a bluish-green tint in the extended halo and at least one region on the edge of the halo of the galaxy. There are no prominent spiral arms or dust lanes visible. Overall, the morphology suggests a galaxy that has largely completed its major star formation phase, with a dominant spheroidal component and an absence of significant ongoing star formation in the central bulge.
