The galaxy presents as a spiral type. The spiral arms are clearly defined, exhibiting a two-armed structure that winds moderately outwards from the central region. Patches of star formation regions are visible along the spiral arms. The central bulge is moderately sized, appearing somewhat bright and yellow-white in color, indicative of an older stellar population. The disk exhibits a slight inclination from our line of sight, providing a view of the spiral structure. There may be some slight distortion and asymmetries. Overall, the galaxy shows some merging history, although it appears largely undisturbed.