The galaxy appears as an elongated, disk-shaped structure, presented almost perfectly edge-on from our perspective. The central bulge region exhibits a bright, concentrated luminosity, suggesting a substantial population of stars. The bulge appears subtly rounded. Dust lanes are visibly obscuring parts of the galaxy's disk, evidenced by darker, patchy regions along the equatorial plane, these features may suggest recent or ongoing star formation activity. The overall color profile indicates a redder hue, implying an older stellar population. The disk appears relatively smooth, lacking distinct spiral arm structures. No signs of tidal tails or major mergers are discernible.
