The galaxy presents a mostly face-on orientation. A central, brighter region suggests a galactic bulge. Faint spiral arms are visible, extending outwards from the central bulge. The arms appear somewhat flocculent and patchy. There appears to be more star formation in the spiral arms that the bulge. Overall, the galaxy exhibits a blue color, suggestive of active star formation. There is no evidence of any major ongoing merger. A slight asymmetry in the outer regions hints at a possible minor gravitational interaction. There may be a weak bar structure in the central region.
