The galaxy appears as an elongated, disk-like structure viewed edge-on. It exhibits a central bulge that is noticeably brighter and yellowish-white in color, suggesting a higher concentration of older stars. Surrounding the bulge is a fainter, bluish disk, indicative of ongoing star formation. The disk appears relatively smooth with some subtle irregularities, possibly due to spiral arm structures that are not clearly resolved at this viewing angle. There are no obvious signs of a major ongoing merger, although there may be minor disturbances present within the disk's structure. The galaxy is moderately distant, with its light being redshifted, indicating its recession velocity. The overall morphology suggests a galaxy with a significant stellar mass and a modest rate of star formation.
