The galaxy presents as an edge-on or highly inclined disk galaxy. There is a central bulge, visibly more concentrated and yellowish in color, suggesting an older stellar population dominating this region. The disk itself appears relatively smooth, exhibiting a gradual decrease in luminosity from the bulge outwards. The bluish color in the outer regions of the disk suggests the presence of younger, hotter stars, indicative of ongoing star formation. The disk appears somewhat asymmetric, with one side appearing slightly more extended than the other. There is some faint evidence of dust lanes within the disk.
