The galaxy appears as a relatively compact object with a smooth, elliptical morphology. It exhibits a concentrated central region with a gradual decrease in luminosity towards its outer edges, indicating a likely spheroid-dominated structure. The galaxy's color is generally redder, suggestive of an older stellar population and reduced ongoing star formation. There is no visible evidence of prominent spiral arms or dust lanes. Overall the galaxy shows minimal signs of recent merger events or significant tidal disturbances.
