The galaxy presents as a highly inclined, disk-shaped structure, likely an edge-on spiral. The central bulge exhibits a rounded morphology with a concentrated luminosity, transitioning to a flattened disk structure. The disk demonstrates a smooth texture, with subtle hints of possible dust lane obscuration along the equatorial plane. Color gradients indicate a potentially older stellar population dominating the bulge, with a shift towards slightly bluer hues along the outer disk, suggestive of ongoing star formation. There is no visually apparent indication of any major mergers or significant tidal disturbances affecting the galaxy's overall morphology.
