The galaxy presents as an edge-on or highly inclined disk galaxy. A prominent central bulge, exhibiting a yellowish-orange hue, dominates the galaxy's core. The disk appears relatively thin and elongated, with a bluer color gradient extending outwards from the bulge, suggesting the presence of younger, hotter stellar populations within the disk. There are hints of possible dust lanes obscuring the central region of the disk, although this is difficult to ascertain definitively from the image. The galaxy does not show any strong signs of significant morphological disturbance or major mergers, appearing relatively undisturbed. There is a suggestion of some faint, diffuse structure extending beyond the main disk, potentially faint tidal tails or an extended stellar halo, but the image resolution limits further analysis.
