The galaxy presents as a lenticular, elongated structure, consistent with an edge-on or nearly edge-on orientation relative to our line of sight. A central bulge is discernible, exhibiting a concentration of light that gradually diminishes outwards. The bulge appears relatively smooth and homogeneous in color, suggesting an older stellar population. The disk component of the galaxy is evident as a flattened structure extending outwards from the bulge. There is a slight blue tinge on the outer edges of the disk, indicating the presence of younger stars within the galaxy. The galaxy displays no signs of major disturbances, suggesting a settled morphology.
