The galaxy presents as an elliptical morphology with a smooth, relatively featureless light distribution. A concentrated central bulge dominates the overall structure, exhibiting a yellowish-orange hue. The surrounding galactic halo appears diffuse and gradually fades into the background sky, indicative of an aging stellar population. There's a subtle elongation, indicating a deviation from perfect sphericity. No distinct spiral arms, bars, or dust lanes are apparent in this imagery. The galaxy appears undisturbed, showing no obvious signs of recent merger activity or tidal interactions.
