The galaxy presents as a spiral type, exhibiting well-defined arms emanating from a central region. Two spiral arms appear to be particularly prominent. The arms are loosely wound, showing significant separation between the spiral arms. There is a noticeable degree of patchiness within the spiral arms, suggesting active regions of star formation. The galaxy is not edge-on; we observe the disk at an oblique angle. The central bulge is of moderate size relative to the disk. There is no visible indication of a strong central bar. No significant morphological disturbances indicative of recent or ongoing major mergers are readily apparent. The overall structure suggests a relatively undisturbed morphology.
