This galaxy presents as a highly inclined, edge-on spiral, with an estimated effective radius of approximately 8.6 kpc. A prominent dust lane bisects the galaxy, obscuring the central bulge region, which appears moderately concentrated, suggesting a classification between a classical and pseudo-bulge. The bulge exhibits a slight boxy morphology. The disk appears thin and relatively smooth, with a visible blue color indicative of on-going star formation. The galaxy shows no obvious signs of a major merger, but there appears to be a minor disturbance or possible satellite galaxy interaction occurring. There is a plume or tidal feature present on the left side of the galaxy indicating a possible tidal interaction.