The galaxy presents as a highly elongated, cigar-shaped structure with a clear major axis. There is a distinct color gradient visible along the primary axis, shifting from a bluish hue at one end to a warmer, reddish tone at the other. This suggests possible variations in stellar populations, dust obscuration, or redshift within the galaxy itself. The morphology indicates an edge-on orientation relative to our line of sight, obscuring any potential spiral arm structure or central bulge.

The overall light distribution is relatively smooth, with a gradual fading of intensity from the center outwards. There are no obvious signs of strong star formation regions or distinct clumps of bright emission. The galaxy appears relatively undisturbed, with no clear indications of major mergers or tidal interactions. Possible minor disturbances might be present, but are hard to discern.
