The galaxy appears to be an elliptical galaxy at a moderate redshift. It exhibits a relatively smooth, concentrated light profile, suggesting an older stellar population. The galaxy's shape is generally round, lacking any distinct spiral arm structures or prominent disk features. There is no obvious evidence of a major merger event or significant tidal disturbances; the galaxy seems relatively undisturbed. The core of the galaxy appears to exhibit a redder hue, likely indicating a higher concentration of older, redder stars. The galaxy's overall color suggests a moderate amount of star formation, though not at a rate indicative of a blue, actively star-forming galaxy. It is a relatively massive galaxy.
