The galaxy presents as a spiral, observed nearly edge-on. A prominent dust lane bisects the galaxy, obscuring the central bulge. The central bulge appears moderately bright and concentrated, displaying a yellow hue. Faint, diffuse spiral arms extend outwards, showing a bluer color, suggesting the presence of younger stellar populations. The overall morphology indicates a disk galaxy with a developed bulge. The color gradient from the central bulge to the outer arms could suggest ongoing star formation. There is a possible interaction between the galaxy and another galaxy. There is a slightly skewed disk, or it could be due to dust, or it could be in the process of merging.
