The galaxy presents as an edge-on spiral. A prominent central bulge is apparent, exhibiting a concentrated, yellowish-orange hue. This suggests an older stellar population within the bulge. Dust lanes are visible, obscuring parts of the disk and contributing to the patchy appearance along its length. The majority of the disk appears relatively smooth, with one area showing a blue tint, possibly indicating recent star formation. Overall, the galaxy shows no major signs of a recent merger or strong tidal interaction.
