The galaxy presents a relatively face-on spiral morphology. Distinct spiral arm structures are visible, with a notable blue coloration suggesting active star formation within these regions. The arms appear somewhat flocculent. The central bulge is not prominently defined, exhibiting a moderate size relative to the disk. There are indications of possible tidal disturbances or interactions, evidenced by asymmetries in the disk and faint extended features. A weak bar structure may be present. Overall, the galaxy exhibits characteristics of a late-type spiral galaxy with ongoing star formation and possible signs of a past or ongoing minor merger event.
