The galaxy presents as an edge-on spiral, exhibiting a distinct disk structure. A central bulge is apparent, displaying a smooth, albeit not perfectly spherical, luminosity profile, which suggests the presence of older stellar populations. The disk itself appears thin and elongated with a relatively high degree of uniformity and a blue tint on the upper edge. Evidence suggests ongoing star formation, particularly towards the edges of the disk. There appears to be some minor disturbances. This could indicate past gravitational interactions.
