The galaxy appears to be a spiral galaxy, observed at a distance corresponding to a redshift of approximately 0.176. It exhibits a well-defined disk structure and prominent spiral arms. The galaxy's morphology indicates that it has two dominant spiral arms. These arms appear tightly wound around the central bulge. The bulge is of moderate size. There is no strong evidence of a bar feature. The disk's light is not uniform but rather patchy, suggesting ongoing star formation within the spiral arms. No significant signs of a major merger are apparent. There are no obvious tidal tails. The galaxy's face is well aligned towards our perspective.
