The galaxy presents a disk morphology with prominent spiral arm structures. These arms appear relatively tightly wound, with a moderate bulge component visible. The overall color suggests a moderate amount of ongoing star formation within the arms. The spiral arms are somewhat asymmetric, indicating a possible gravitational interaction. The central region is slightly brighter and exhibits a yellowish hue, potentially indicative of an older stellar population concentrated in the bulge. The disk is not perfectly edge-on, allowing for a clear view of the spiral structure. There are indications of minor disturbances in the disk, and there are hints of tidal features suggestive of previous or ongoing interactions.
