The galaxy presents as a spiral galaxy with a moderate bulge. The spiral arms are prominent and extend outwards from the central bulge, displaying a relatively high degree of organization. There's a suggestion of a bar structure, but it is not overly distinct. The disk is oriented at a shallow angle to our line of sight. The color profile of the galaxy indicates that it is composed of a mix of older stellar populations within the central bulge and disk, and younger, blue stars residing within the spiral arms. It shows no obvious signs of any major or minor mergers.
