The galaxy presents a morphology consistent with a spiral galaxy, viewed at an angle that is not quite face-on, but not fully edge-on either. Prominent spiral arms are visible, emanating from a central bulge region. The bulge appears relatively small. The spiral arms display a winding pattern, appearing moderately tightly wound around the center of the galaxy. Two main arms are discernible, exhibiting some patchiness, possibly indicating areas of active star formation. Overall, the galaxy does not appear to be undergoing a major merger or significant tidal disturbance, although there may be a slight asymmetry or minor disturbance in one of the arms. There does not appear to be a strong bar feature bisecting the central bulge. The galaxy appears to be a late-type spiral galaxy, with a notable disk component and relatively less emphasis on the bulge.
