The galaxy presents as a spiral type, exhibiting a distinct, yet somewhat tightly wound, spiral arm structure. The spiral arms are relatively thin and feature a noticeable blue hue, suggesting ongoing or recent star formation activity.

A prominent central bulge is observed, appearing bright and somewhat diffuse. The bulge seems to have a moderate size compared to the overall disk. There's evidence of a bar-like structure crossing the central region, although it does not appear particularly pronounced. 

Overall, the galaxy's disk is viewed at a slight angle, but not completely edge-on. There may be moderate disturbances occurring, and a relatively high fraction of recent star formation is visible.
