The galaxy exhibits a distinct disk morphology with visible spiral arm structures. The arms appear tightly wound and there is a prominent bulge. The galaxy is observed at a moderate inclination, allowing partial visualization of the spiral arms. A bar structure may exist traversing its central region. Based on the morphology there may be a minor gravitational interaction with a neighboring galaxy. The disk demonstrates a bluer color profile in its outer regions, suggesting ongoing star formation. The central bulge region exhibits a yellow-red hue, potentially indicative of an older stellar population.
