The galaxy presents as a spiral type, exhibiting a discernible disk structure. Two prominent spiral arms are visible, winding moderately outwards from the central region. The arms display a mix of blue hues, suggesting ongoing star formation within them. The central bulge appears relatively small in comparison to the overall disk size. While the bulge is somewhat smooth, the spiral arms show some patchiness, possibly indicating regions of differing stellar densities or obscured dust lanes. There may be a weak bar structure in the center. No obvious signs of a major merger are apparent, although there may be a minor disturbance. Overall, the galaxy appears to be relatively face-on.
