The galaxy presents as a relatively small, elongated, cigar-shaped structure. Its light distribution appears smooth with no distinct features such as spiral arms or a prominent central bulge visible in this image. The color is generally blueish-white, suggesting a stellar population that is relatively young, with at least some ongoing star formation. There is no obvious dust lane visible through the galaxy, although the resolution may be insufficient to confirm this. There is no sign of any tidal tail or other evidence of a major merger, although there are some signs of a minor disturbance. The galaxy's structure and colour profile implies a disk-like morphology, seen from an edge-on perspective.
