The galaxy presents as an edge-on spiral, exhibiting a prominent central bulge. The bulge appears smooth and somewhat elongated along the major axis of the galaxy. A disk is visible, but due to the edge-on orientation, detailed structural features such as spiral arms are not discernible. The galaxy's light profile suggests a concentration of older stellar populations, especially within the bulge. A slight blue hue can be seen along the outermost parts of the disk, though it is subtle. There is no sign of a major merger but subtle irregularities within the disk suggest minor disturbances. The galaxy appears relatively isolated.
