The galaxy presents a generally smooth, elliptical morphology. Its light is centrally concentrated, exhibiting a bright core region that gradually fades toward the outer edges. There is little evidence of distinct spiral arms or significant substructure within the galactic disk; overall the galaxy appears to be relatively undisturbed. The galaxy's color is primarily characterized by a redder hue, suggesting an older stellar population with lower star formation rate. Based on its redshift value, this is a distant galaxy.
