The galaxy appears to be a spiral, although its structure is somewhat disrupted. The spiral arms are discernible but not well-defined, exhibiting a clumpy morphology with regions of enhanced blue luminosity indicative of recent star formation. There is no obvious central bulge, and if one exists it's likely very small. The overall color suggests an actively star-forming galaxy, but that it is also in the early stages of merging with another smaller object or experiencing some other form of gravitational interaction.
