This galaxy exhibits a flattened, disk-like morphology, appearing almost edge-on from our vantage point. A central bulge is visible, exhibiting a yellowish hue, which suggests an older stellar population. The disk itself shows a bluer color gradient moving away from the bulge, indicative of ongoing star formation within the spiral arms. There appear to be some disturbances within the structure of this galaxy, however these are minor. The galaxy is relatively small and has a low Sersic index, meaning it is likely a disk dominated galaxy with a weak bulge. The faintness of the disk also suggests a relatively low stellar mass.