The galaxy presents as a face-on spiral with a prominent central bulge. The bulge exhibits a yellow-orange hue, suggesting an older stellar population. Distinct spiral arms are visible, characterized by a blue tint, indicative of ongoing star formation. These arms are somewhat tightly wound around the bulge. The galaxy displays a moderate disk with some irregular structure, hinting at possible gravitational interactions or internal disturbances. There is no strong evidence of a central bar. Overall, the galaxy appears relatively undisturbed, although the spiral arms suggest some past or present interaction.
