The galaxy presents as a grand design spiral with two prominent, tightly wound spiral arms. The arms emanate from a bright, moderately sized central bulge, which contributes significantly to the galaxy's overall luminosity. The color gradient suggests an active star forming region. There are minor disturbances, or an irregular component, in the outer disc regions. No significant bar structure is apparent. The galaxy appears relatively isolated, showing no obvious signs of major interaction or merging. The galaxy disk is oriented face-on.
