The galaxy presents as a spiral, observed nearly edge-on. A dust lane is visible, bisecting the galaxy's elongated form and obscuring the central bulge. The disk appears relatively smooth with no distinct spiral arm structure discernible at this resolution, though a slight asymmetry is visible along the plane of the disk. The overall color is somewhat blue, especially in the areas extending outwards from the central bulge. This suggests the presence of recent or ongoing star formation. There is no obvious evidence of a major merger or tidal disturbances. The galaxy appears to be relatively isolated, with no immediate companion galaxies.
