The observed galaxy presents as a spiral galaxy, viewed at an angle that is moderately inclined relative to our line of sight. The spiral structure is clearly visible, exhibiting primarily two distinct arms. These arms appear somewhat tightly wound. Evidence suggests the presence of a central bulge, of a moderate size. The presence of a bar feature is also indicated. There is no apparent sign of major ongoing merger activity, although some minor disturbances may be present in the galaxy's morphology. The galaxy has a distinct disk-like appearance.
