The galaxy presents a discernible disk structure, exhibiting prominent spiral arms. The winding of these arms appears to be primarily tight to medium in nature. Two arms seem to be the dominant feature. The central bulge is evident, appearing to be of moderate size. The overall color profile suggests active star formation, with bluer regions interspersed within the spiral arms. There are no obvious signs of a strong bar feature. Some evidence of minor disturbances are visible in the disc morphology.
