The observed galaxy presents as an edge-on spiral, exhibiting a clearly defined disk. The dominant color appears to be reddish-orange. The bulge region is distinctly prominent and elongated. While it seems smooth in texture, there may be a degree of boxiness to the bulge, and shows a more rounded shape. There is some indication of disturbance along the plane of the disk. The galaxy exhibits a moderately high rate of star formation and a significant stellar mass. There is no clear sign of a recent major merger, although there are signs of minor disturbance within the galaxy.
