The galaxy presents as a well-defined, elongated structure. It exhibits a smooth, centrally concentrated luminosity profile, suggesting a relatively evolved stellar population. The galaxy's shape is markedly cigar-shaped.  Faint blue tinges along the edges hint at some ongoing star formation. There is no evidence of a major ongoing merger. Faint disturbances are present. Overall, the galaxy's morphology indicates a possible late-type spiral galaxy, seen edge-on.
