The galaxy appears to be a spiral galaxy viewed almost completely edge-on. A prominent dust lane bisects the galaxy's disk, obscuring the central bulge. The disk appears relatively smooth, lacking distinct spiral arm structures. The galaxy's color profile suggests a population of older stars, with a slight bluish tint in the outer disk potentially indicating some ongoing star formation. The bulge appears moderately sized and slightly boxy in shape. There is no evidence of strong tidal distortions or major mergers. There might be a faint indication of a minor disturbance in the galaxy's disk, potentially due to a past interaction.
