The galaxy presents as a spiral type, appearing nearly face-on relative to our line of sight. It exhibits a moderately sized bulge that is bright white, with a gradual decrease in luminosity towards the outer regions. The spiral arms are clearly defined and wind tightly around the central bulge. HII regions appear sparse in the spiral arms. The galaxy exhibits a moderate amount of blue coloration, suggesting ongoing though not vigorous star formation. There is no evidence of a strong bar feature. The galaxy displays an overall well-defined structure with no major signs of tidal disturbances or ongoing major merging events.
