The galaxy exhibits a disk-like structure with a prominent central bulge. The bulge appears yellowish-white, suggesting an older stellar population. The disk component has a distinct spiral structure, exhibiting multiple arms emanating from the central region. These spiral arms display a mix of bluish and reddish hues, which indicates both young star formation and older stellar populations. The spiral arms are moderately wound, neither tightly coiled nor very loose. There is some evidence of a bar-like structure across the central region, although it is not very pronounced. The overall shape is slightly elliptical, with a high degree of symmetry, and there is no obvious sign of recent merger activity or major disturbance. The galaxy is observed at a redshift indicating a substantial distance, thus the finer details are blurred.
