The galaxy appears to be a spiral galaxy, observed at a redshift of approximately 0.165. The galaxy presents a disk-dominated morphology, with spiral arms clearly visible. These arms are moderately wound around a central bulge. The bulge size relative to the disk appears to be moderate to small. The spiral arms exhibit a flocculent structure, with patches of star formation regions. A bar-like feature is present within the central region of the galaxy, possibly of intermediate strength. There is no obvious evidence of a major merger or tidal disruption. The general shape and structure suggest a galaxy undergoing normal spiral evolution.