The object appears to be a spiral galaxy viewed nearly edge-on. The galactic disk exhibits a distinct flattening. A central bulge is visible, presenting a somewhat rounded morphology, with a moderate concentration of light compared to the disk. The disk component shows evidence of dust lanes, particularly along the plane of the galaxy. A faint, diffuse halo is potentially present. There may be subtle tidal features or minor disturbances indicating interaction with other galaxies, but the overall structure is not largely disrupted. There does not appear to be a presence of strong, active star formation. 
