The observed galaxy presents as a spiral type, with a generally disk-shaped morphology that is not viewed perfectly edge-on. Distinct spiral arm structures are visible, though somewhat loosely wound. The arms appear moderately populated with regions that may represent areas of active star formation. A central bulge is present; its size appears moderate relative to the overall disk. The bulge exhibits a smooth, relatively featureless appearance, contrasting with the more structured arms. There is no obvious evidence of a strong bar structure, nor is there any pronounced indication of a major ongoing merger or strong tidal disturbance of its structure.
