The galaxy appears to be a spiral galaxy, viewed at an oblique angle, not quite edge-on. It exhibits a discernible disk structure with evidence of spiral arms. The spiral arms are somewhat tightly wound and present a two-armed structure. The central bulge is visible, it appears small to moderate in size, with a concentrated central region. The color profile suggests a mix of stellar populations. The bulge shows a slightly redder hue, potentially indicating older stars, while the disk displays bluer regions consistent with ongoing star formation within the spiral arms. There appears to be no strong evidence of a prominent bar structure. Overall, the galaxy presents a relatively undisturbed morphology.
