The galaxy presents as a moderately bright, resolved object. It appears elliptical in shape, displaying a smooth, featureless morphology across its visible extent. There's a noticeable color gradient, transitioning from a slightly bluer hue in the central region to a redder periphery. This suggests potential differences in stellar populations or dust content across the galaxy's structure, with possibly younger, bluer stars concentrated in the core, and older, redder stars dominating the outer regions. The lack of discernible spiral arms or distinct features indicates a classification likely leaning towards an early-type galaxy. Faint extensions or tidal features are not readily apparent in the image, suggesting a relatively isolated system with no recent major merger events.
