The galaxy exhibits a disk-like morphology, with visible spiral arm structures. The arms appear somewhat flocculent, with multiple regions of star formation evident as localized brighter areas, particularly in the bluer wavelengths. The central bulge is moderately sized, not dominating the overall galaxy profile. There is no strong central bar structure, but a subtle elongated feature might indicate a weak bar. No major disturbances or signs of an ongoing merger are readily apparent. The galaxy is primarily blue, possibly indicating ongoing star formation throughout. The structure is not perfectly smooth; the disk shows some clumpy features and asymmetries.
