The observed galaxy presents a spiral structure. The arms appear relatively well-defined and extend outwards from a central bulge. The bulge exhibits a moderate concentration of light. Some indication of faint bar structure might be present. The spiral arms contain several regions that display a clumpy, star-forming morphology. The overall color of the galaxy suggests ongoing stellar formation activity, particularly in the arms, while the bulge appears more yellow and consistent with an older stellar population. The galaxy exhibits a disk component with a tilted orientation relative to our line of sight. A hint of an edge-on disk can be observed with some warping. Evidence for a minor disturbance or potential interaction is weakly present.
