The galaxy presents as a strongly edge-on spiral, exhibiting a highly elongated, disk-like structure. A prominent central bulge is apparent, displaying a concentrated yellowish-orange hue indicative of an older stellar population. The disk is very thin and shows hints of blueish hues at the edges, possibly indicating younger, hotter stars and regions of ongoing star formation. The dark dust lanes appear as subtle but noticeable, indicating the presence of interstellar dust obscuring the light from stars behind it. Overall, the galaxy presents a relatively smooth and undisturbed appearance, without any obvious signs of major mergers or interactions.
