The galaxy presents as an elongated, edge-on spiral, exhibiting a distinct disk structure. The central bulge appears prominent, displaying a yellowish-orange hue, suggestive of an older stellar population within this region. The disk, extending outwards from the bulge, shows bluer colors, indicative of ongoing star formation. A dust lane appears present, bisecting the galaxy's disk, though is indistinct. There is no obvious distortion of the galactic shape. No signs of any merging or interactions are evident.
