The galaxy presents as a spiral galaxy with a prominent disk structure. The spiral arms are well-defined, displaying a moderate winding pattern. Two distinct arms are visible, emerging from a central bulge. There are multiple prominent regions of star formation in the spiral arms, which give them a somewhat clumpy and irregular appearance, indicating active star formation. The central bulge appears relatively small and not particularly luminous, suggesting it is not a dominant feature of the galaxy. There is some evidence of a bar-like structure running through the center of the galaxy, although it is not sharply defined. The galaxy appears relatively undisturbed, with no obvious signs of a major merger event, though some minor tidal features or disturbances cannot be ruled out. The galaxy is observed at redshift of 0.265272, which places it at a significant distance from us and is responsible for the observed colour shift. The estimated size is approximately 9.17 kpc across.