The galaxy presents as a fairly luminous object at a redshift of approximately 0.216, indicating a considerable distance. Morphologically, it exhibits characteristics leaning toward a smooth structure with some intermediate rounding. There isn't a strong indication of significant disk features or spiral arms. The core displays a concentration of light, suggesting the presence of an older stellar population. The galaxy appears to be in a relatively isolated state with only minor disturbances to its structure, implying an absence of recent major merger events. There is a weak level of star formation detected in the galaxy. Overall, the galaxy appears as a massive but relatively passive system.
