The galaxy presents as a disk-shaped structure viewed nearly edge-on. A prominent central bulge is visible, exhibiting a smoother, more concentrated luminosity profile compared to the outer disk. The disk shows evidence of dust lanes, appearing as dark and irregular bands obscuring the light from stars behind them. The colour gradient suggests a redder hue at the centre, which becomes bluer towards the outer edges, possibly indicating a larger population of younger stars. There is no visual indication of major mergers or significant tidal disturbances. The galaxy appears to be a relatively undisturbed system undergoing steady star formation.