The galaxy presents a discernible spiral structure. Two prominent spiral arms are clearly visible, emanating from a central region that exhibits a moderately sized bulge. The winding of the spiral arms appears primarily of medium tightness, suggesting a balanced gravitational influence. The overall form of the galaxy is not perfectly symmetrical, potentially indicating minor gravitational interactions or internal disturbances. There does not appear to be a strong central bar feature. The galaxy appears to have some diffuse, less condensed regions of star formation.
