The galaxy appears as a relatively compact object with a smooth, elliptical morphology. It exhibits a primarily rounded shape. There seems to be little or no evidence of spiral arm structure or significant dust lanes, consistent with it being an early-type galaxy. The color gradient suggests a concentration of older stellar populations, particularly at the core. I observe a distinct core with a concentrated luminosity profile, which is surrounded by a more diffused halo of light. I see no signs of major disturbances or active galactic nuclei within the visual field. The galaxy's overall color is slightly redder than the surrounding background, suggesting that the dominant stellar population has evolved. There seems to be a slight merging or tidal stream, indicated by the minor disturbance.
