This galaxy appears to be a spiral galaxy, viewed at a slight angle relative to face-on. There is evidence of spiral arm structure, but they appear somewhat flocculent and not tightly wound. A central bulge is visible, appearing of moderate size. The disk of the galaxy shows distinct blue regions, indicating ongoing star formation, possibly concentrated along the spiral arms. There is no clear evidence of a strong bar structure. The overall morphology suggests a galaxy experiencing active star formation within its disk, but without strong indications of recent major merger events. The object appears as a disk galaxy that is neither totally smooth nor strongly disturbed.
