The galaxy presents as a spiral morphology, exhibiting prominent, well-defined arms. The spiral arms appear grand design, with a clear two-arm structure that originates near the central bulge region. The arms show moderate winding, not overly tight or loose, with a flocculent texture along their length. The central bulge is of moderate size relative to the disk, appearing luminous with a yellow hue, suggesting a concentration of older stellar populations. No strong bar structure is visible, though a subtle, elongated density enhancement might be present. The disk is oriented approximately face-on relative to our line of sight. There is no obvious sign of tidal disturbances or major mergers. The spiral arms show blue regions indicating star formation. The galaxy exhibits a smooth overall appearance.