The galaxy presents as a spiral type, viewed at an angle, with spiral arms clearly visible. A central bulge is present, though it appears relatively small in comparison to the overall disk size. The dominant color is a bluish hue, suggesting active star formation is ongoing. There's an irregular distribution of light within the disk, with areas of enhanced brightness which could be due to more intense star forming regions. Overall, the galaxy appears well-defined, with no obvious signs of major interactions or merging, though there is possibly a minor disturbance. The galaxy is more disk dominated rather than bulge dominated. There is a weak bar structure in the center of the galaxy.
