The galaxy presents a relatively smooth, symmetrical morphology. The light distribution appears centrally concentrated, showing a gradual decrease in intensity from the core outwards. A slight elongation is discernible, but the galaxy maintains a largely round shape. The color profile suggests a redder hue. This implies an older stellar population and/or significant dust obscuration. There is no obvious presence of spiral arms or prominent star-forming regions. No major disturbances or signs of ongoing mergers are apparent. A minor, very slight, asymmetry can be perceived. Overall, the galaxy appears as a relatively passive system, likely an elliptical or lenticular galaxy at moderate redshift.
