The galaxy presents as a spiral type, exhibiting a disk-like morphology. There is evidence of flocculent spiral arm structure. A bar is visible across the central region of the galaxy, appearing relatively strong. The bulge of the galaxy is moderately sized, contributing a substantial fraction of the galaxy's overall luminosity. The winding of the spiral arms appears primarily medium. There is no visually obvious sign of any major merging activity or tidal distortions. The galactic disk is not seen edge-on; the view is nearly face on.
