The galaxy presents as a face-on spiral, characterized by two prominent spiral arms emanating from a central bulge. These arms exhibit a moderate winding pattern, appearing neither tightly wrapped nor excessively loose. The arms show a distinctly blue hue, potentially indicative of active star formation regions within. The central bulge appears moderately sized, with a yellowish coloration. The overall structure suggests a classic spiral galaxy morphology. Evidence points to a system that is largely undisturbed, without signs of a major galactic merger. The galaxy appears to be relatively massive, as evidenced by its luminosity and size.