The galaxy presents as a spiral galaxy, observed at an inclined angle. The central bulge appears prominent, exhibiting a yellowish hue, suggesting an older stellar population. The spiral arms are well-defined, and wind tightly around the bulge. They are populated with bluer regions indicating ongoing star formation. There is a noticeable dust lane structure within the spiral arms, adding to their patchy appearance. The overall structure suggests a grand design spiral with a possible bar feature across the central bulge. Faint diffuse outer regions are visible extending beyond the main spiral structure. The galaxy does not show signs of major tidal disturbances.
