This galaxy appears to be a spiral galaxy, viewed nearly edge-on. The central bulge is prominent and elongated, exhibiting a smooth, concentrated appearance with a yellow-white hue, suggesting an older stellar population. The disk component is flattened and extends outwards from the bulge, with a slight warp that gives it a somewhat irregular shape. Dust lanes are not clearly visible, which suggests the galaxy has either a low dust content or the angle of inclination is obscuring their detection. Given the apparent smoothness of the disk, star formation may be relatively quiescent at this time. The galaxy's color indicates it is likely a moderate mass galaxy at an intermediate redshift. The lack of tidal features suggests that it is not undergoing a recent major merger, although minor disturbances may be present. The overall shape is generally consistent with a classic edge-on spiral morphology.
