The observed galaxy presents a disk-like morphology, oriented approximately edge-on with respect to our line of sight. A central bulge region is discernible, though not particularly prominent. The galaxy appears to exhibit a flocculent spiral arm structure, although the tight winding of these arms makes it difficult to clearly distinguish individual arms. The overall color of the galaxy is yellowish-white, potentially indicating a population of older stars. There are no obvious signs of a strong central bar structure. The galaxy appears relatively undisturbed, lacking any significant indications of recent or ongoing major merger activity. There might be minor disturbances in the disk.
