The galaxy presents as an edge-on or highly inclined spiral. A prominent central bulge dominates the core region, exhibiting a smooth, concentrated light profile. This suggests a high density of older stellar populations within the bulge. Faint, extended galactic disk spans approximately three times the diameter of the bulge along its major axis. It has a smooth texture, and no distinct features such as spiral arms or dust lanes are obviously apparent. Overall the galaxy exhibits a somewhat diffuse appearance, with no signs of current or recent major mergers.
