The galaxy presents a smooth, elliptical morphology with a centrally concentrated light profile. There is a lack of distinct spiral arm structures or prominent dust lanes, indicating a relatively passive or quiescent state of star formation. The overall color appears to be slightly yellow-redder than the foreground objects which suggests a population of older stars, with a possible contribution from dust reddening. The galaxy is elongated, showing an elliptical shape and a bright core. There's no strong evidence of recent merger activity or tidal disturbances in the galaxy's structure. The galaxy's luminosity appears substantial, consistent with a relatively massive galaxy at its redshift. 
