The galaxy presents as a spiral type. The structure exhibits a central bulge of moderate size, characterized by a yellowish hue. Two prominent spiral arms emanate from the central region and are easily discernible. The arms are not tightly wound, and a medium winding grade is present. These arms display noticeable knots of star formation, evidenced by their bluer color. The disk is face-on, and no signs of significant interactions or major disturbances with other galaxies are present; however, the image indicates a potentially minor disturbance. A strong bar-like structure is present across the galactic center. Overall, the galaxy appears actively forming stars within its spiral arms.
