The galaxy appears to be a spiral galaxy, exhibiting well-defined spiral arms. The arms are somewhat loosely wound and display a clumpy structure, suggesting regions of active star formation. The color is predominantly blue, especially within the arms, also indicative of ongoing star formation. A central bulge is visible, appearing yellowish in color, implying an older stellar population. The bulge is relatively small in comparison to the overall size of the disk. There are no signs of any major mergers or strong tidal disturbances. The galaxy's disk is oriented at a significant angle relative to our line of sight, but not perfectly edge-on. There is no strong bar structure visible.
