The galaxy presents as an edge-on or highly inclined disk galaxy. A prominent central bulge dominates the visual structure. The bulge exhibits a smooth, rounded morphology, with a yellowish-orange color, indicative of an older stellar population. The galactic disk appears relatively thin and exhibits a bluer hue than the bulge, suggesting the presence of younger, hotter stars and possibly ongoing star formation. There's a hint of dust lane obscuring the central region of the disk. The overall structure doesn't indicate any major tidal disturbances or ongoing merger activity.
