This galaxy presents as a relatively smooth, disk-like structure viewed edge-on. A faint central bulge is observable, exhibiting a slightly redder hue compared to the rest of the disk. The disk itself appears to be composed of diffuse, bluish light, suggestive of ongoing or recent star formation. There's no obvious dust lane obscuring the central regions, but a slight attenuation of light is possible along the major axis. The outer edges of the galaxy are less defined and seem to fade into the background sky. The overall symmetry of the galaxy is relatively undisturbed, showing no signs of major mergers or tidal distortions. There is no visible active galactic nucleus. The galaxy appears to be a relatively isolated system.
