The galaxy appears to be a spiral galaxy, viewed at a slight angle. The central bulge is prominent and exhibits a yellowish hue, suggesting an older stellar population. Faint spiral arms extend outward from the bulge. These arms display hints of bluer regions, potentially indicative of ongoing star formation. The arms are moderately tightly wound and somewhat difficult to discern completely, blurring into each other. The overall structure suggests a barred spiral galaxy. The disc shows slight signs of minor disturbance, possibly due to a recent interaction. Overall, the galaxy exhibits a mixed morphology, with a notable bulge component and discernible spiral arms.
