The galaxy presents as a spiral type, with a notable disk structure. The spiral arms appear grand design, exhibiting a prominent two-armed morphology. They are moderately wound. The bulge component is of moderate size relative to the disk. There's no clear evidence of significant tidal disturbances or ongoing major mergers, although the galaxy appears somewhat asymmetrical, possibly indicative of a minor interaction or internal dynamics. There appears to be a weak bar running through the galaxy.
