The galaxy presents as a generally smooth, centrally concentrated object with a round morphology. The light distribution appears relatively uniform, suggesting a lack of prominent spiral arms or distinct substructures. A slight color gradient is observable, transitioning from a yellowish central region to a redder hue in the outer regions. No obvious signs of tidal disturbances or merging activity are apparent from visual inspection. The overall impression is that of an elliptical or lenticular galaxy, potentially a passively evolving system.
