This galaxy presents as a well-defined spiral structure, exhibiting prominent arms. These arms extend outwards from a central, moderately-sized bulge. The spiral arms appear open, with a loose winding pattern. Evidence suggests two major arms dominate. A bar structure may be present, but it is not definitively strong. The overall morphology indicates the presence of a disk, viewed at a slight inclination. The galaxy displays signs of active star formation, particularly within the spiral arms, based on color gradients. No signs of significant tidal disruption or ongoing major merger activity are visible, though minor disturbances cannot be ruled out.
