The galaxy exhibits a disk-like structure, presented at an almost edge-on orientation relative to our line of sight. A distinct central bulge is observed, appearing brighter and more concentrated than the surrounding disk. The disk appears to be smooth, without obvious spiral arm structures, suggesting a relatively high degree of organization. Some indications of slight disturbances may be present. The colour of the disk and bulge suggest ongoing star formation activity, with a general blue-white tinge to parts of the disk that likely indicates areas of more recent, or higher, star formation, while the bulge appears more yellow, which could indicate an older stellar population. Overall the galaxy appears to be a relatively undisturbed disk galaxy.
