This galaxy appears to be an edge-on spiral, exhibiting a disk-like structure oriented nearly parallel to our line of sight. There is a prominent central bulge, appearing smooth and somewhat rounded. The disk itself shows some signs of internal structure with some minor disturbances, but there are no signs of active merging with another galaxy. There appears to be a dust lane running through the center of the galaxy, but the image is not clear enough to fully resolve it. The galaxy displays a color gradient, with the central bulge appearing more yellowish, suggesting an older stellar population, and the outer disk having a hint of bluer hues, indicating the presence of younger, hotter stars. 