The galaxy presents as a spiral type, exhibiting a prominent disk structure. A distinct, elongated bar feature bisects the galactic nucleus, oriented approximately horizontally in the frame. Two well-defined spiral arms emanate from the ends of the bar, tightly wound around the galactic center. The arms display a somewhat flocculent structure, with noticeable clumping of brighter regions indicating areas of active star formation. The bulge component appears to be relatively small. There is a slight asymmetry to the structure of the outer disk, particularly on the left side of the frame. There is no obvious indication of major mergers or strong tidal interactions, though some minor irregularities may exist. Overall, the galaxy seems to be well-defined in its spiral structure, presenting a relatively standard example of a barred spiral galaxy at this distance.
