The galaxy presents as a thin, elongated structure, with an apparent high degree of inclination relative to the observer's line of sight. The light distribution suggests a higher concentration of stellar density towards the central region, which is likely a galactic bulge. The overall color is bluish, possibly indicating the presence of younger stellar populations and ongoing star formation within the disk. There is little evidence of spiral arm structure due to its edge-on orientation. The galaxy appears relatively undisturbed, showing no obvious signs of major mergers or tidal interactions.
