The galaxy presents as a spiral with well-defined, prominent arms. These arms exhibit a relatively organized structure. There appears to be a central bar-like feature spanning a considerable length across the galaxy's core region. The bulge appears to be moderate in size relative to the disk, with the outer disk extending notably beyond the bulge region. The galaxy disk shows no significant disruption or signs of a recent major merger. Star formation appears to be taking place throughout the disk and spiral arms.
