The observed galaxy presents as a spiral, viewed edge-on. Dust lane obscuration is prominent, bisecting the galaxy's primary axis and contributing to a reddish hue in the galactic plane. A central bulge is visually discernible but not particularly prominent. There does not appear to be any signs of merging or tidal disturbances. The galaxy exhibits a moderate degree of symmetry. Based on the colors, there is evidence of star formation, primarily in the central region. 
