The galaxy presents as a late-type spiral, viewed nearly edge-on. A prominent dust lane bisects the galaxy's disk, absorbing light from the stars behind it. The central bulge appears somewhat elongated along the major axis, exhibiting an oval shape with a more rounded structure. Star formation appears present, with visible patches of bluer light interspersed within the disk. There is no obvious evidence of a major ongoing merger or significant tidal distortion, though the galaxy's asymmetry warrants closer inspection for minor disturbances. 
