The galaxy presents as a smooth, elongated structure, possibly a lenticular or elliptical galaxy viewed at an angle. It has a relatively high level of uniformity in surface brightness across its structure, suggesting a lack of significant spiral arms or distinct features associated with active star formation. The galaxy core shows a bright, concentrated luminosity, indicating a central region of high stellar density. Its cigar shape could point towards a morphological classification of an elliptical or S0 galaxy seen edge-on, though the lack of a clear dust lane makes it unlikely to be spiral. There appear to be no signs of ongoing major mergers or tidal disruptions.