The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge that appears bright and gradually diffuses outwards into a fainter halo. The shape is predominantly round, with minimal deviation from a circular form. There is a subtle color gradient, the central region appears slightly yellower/whiter, transitioning to a bluer hue in the outer regions, suggesting some ongoing, low-level star formation, even though the general morphology points towards an older stellar population. There are no apparent signs of significant disturbances or mergers; the galaxy seems settled and undisturbed. The absence of well-defined spiral arms or a prominent disk structure further supports its classification as an elliptical galaxy.
