This galaxy presents as a highly elongated, disk-shaped system viewed at a steep angle. The central region exhibits a concentrated luminosity, appearing yellowish-white, suggestive of an older stellar population. Extending outwards from this central bulge, the disk displays a bluer hue, indicating the presence of younger, hotter stars and potential star forming regions. The edges of the disk are less well-defined, fading gradually into the background, with no obvious spiral arm structure visible. There are no obvious signs of mergers or major tidal disturbances. The object appears relatively undisturbed with a smoothly distributed light profile.
