The galaxy presents as a slightly inclined spiral structure. Two well-defined spiral arms are visible, extending from a moderately sized central bulge. The winding of these spiral arms appears intermediate, neither tightly wound nor exceptionally loose. A central bar structure is not readily apparent. The disk of the galaxy exhibits a mottled texture, suggesting ongoing star formation. There is no clear visual evidence of a major merger, however, some minor irregularities in the disk hint at a potential past interaction. The bulge is yellow in color, with blue tinges outlining the spiral arms.