The galaxy presents a distinct spiral morphology. Several spiral arms, displaying varied winding tightness, emanate from a central region. The arms themselves appear relatively well-defined, though with some flocculence, showing regions of active star formation. The central bulge appears moderate in size, transitioning smoothly into the spiral arms. The lack of significant asymmetry in the disk suggests no major ongoing merger events, although there is some slight distortion in the spiral arms that may indicate a minor interaction. A faint bar structure is suggested, as the central bulge appears slightly elongated.
