The galaxy presents as a bluish, moderately sized object. Its morphology appears somewhat irregular, lacking a well-defined spiral structure. The light distribution suggests a concentration toward the center, which could indicate a central bulge or active galactic nucleus. Some clumpy regions of brighter emission are visible within the disk, likely indicating regions of active star formation. The overall color and irregular structure suggest a galaxy that might be in a phase of active evolution or potentially experiencing gravitational interaction.
