The galaxy appears to be an edge-on spiral galaxy, exhibiting a flattened, disk-like structure. The central bulge is prominent and appears to be spheroidal in shape. The light distribution is dominated by redder wavelengths, suggesting an older stellar population within the bulge. The galaxy has an apparent smooth morphology with little evidence of strong spiral arm structure. There appears to be faint dust lane present, obscuring light in a region near the midplane of the disk. Given the disk's orientation, morphological disturbances such as tidal tails or warped disks are subtle or absent. Overall, the galaxy appears to be a relatively undisturbed, mature spiral galaxy.
