The galaxy presents as a spiral type, exhibiting a disk structure with a noticeable inclination relative to the line of sight. The spiral arms are well-defined, tightly wound around the galactic center, and traceable throughout a significant portion of the disk. Multiple arms appear to be present, showing some bifurcations.

A central bulge is apparent, characterized by a concentrated luminosity which is a moderate size compared to the rest of the galaxy. There is no clear evidence of a strong bar structure bisecting the bulge region.

The overall appearance suggests a relatively undisturbed morphology. There is no strong evidence of ongoing major merger activity.
