The galaxy presents as a spiral type, exhibiting a disk-dominated morphology. Prominent spiral arms are visible, emanating from a central bulge. A strong bar structure traverses the core region. The spiral arms display a winding pattern transitioning from medium to loose as they extend outwards. The bulge component appears to be moderate in size relative to the overall galactic structure. The color profile suggests active star formation within the spiral arms and disk region. There are no visible signs of major mergers or significant disturbances in the galactic structure, though some minor disturbances cannot be ruled out.
