The galaxy presents as an edge-on spiral system. The disk exhibits a high degree of inclination relative to our line of sight. Dust lanes appear prominent within the galactic plane, obscuring the starlight and giving a mottled appearance. The central bulge is visible, appearing somewhat elongated and with a color index that indicates an older stellar population, suggesting a lack of recent star formation in the bulge region. The overall morphology suggests a relatively massive system, likely a late-type spiral galaxy. There is no obvious major interaction, but it looks like it may have a minor disturbance.
