The galaxy appears as an elongated, elliptical structure with a smooth, diffuse light distribution. There is no clear evidence of spiral arms or a prominent disk. The light is concentrated toward the center, suggesting a high degree of central mass concentration. The galaxy has a moderate redshift, suggesting it is relatively nearby. Based on its appearance, the galaxy is likely an elliptical galaxy with low ongoing star formation. No tidal tails or signs of recent major merger events are apparent, although there might be some minor disturbances within the galaxy's structure. The color profile shows a gradient that is redder toward the center.
