The galaxy appears to be a spiral galaxy viewed nearly edge-on. A prominent central bulge is visible, exhibiting a smooth, concentrated light profile suggestive of an older stellar population, likely consisting of evolved red giant stars. This bulge is surrounded by a relatively thin, elongated disk. The disk shows a slight blue tint along its edges indicating younger stars within the spiral arms. There are no other disturbances, such as tidal tails, major asymmetries, or signs of recent mergers.
