The galaxy appears to be a spiral galaxy, presenting a face-on orientation relative to our line of sight. Its structure reveals a prominent central bulge, which is moderate in size and emits light with a yellowish hue. The spiral arms are well-defined and exhibit a relatively tight winding pattern. The disk component shows a blue color, with some apparent star formation. The spiral arms appear to branch and divide, suggesting a multi-armed morphology. No significant disturbances or signs of recent major merger events are readily apparent. There is no clear evidence of a strong bar-like structure within the central region. The overall morphology suggests a relatively isolated galaxy that is actively forming stars within its spiral arms.
