The galaxy presents as a spiral type, with a notable bulge component. Spiral arms are visible, though somewhat tightly wound. The galaxy exhibits an overall moderate inclination relative to our line of sight, but we are not quite viewing it edge-on. There is a suggestion of a bar structure bisecting the central bulge, albeit subtle. The galactic disk shows evidence of spiral structure and some asymmetry. The light distribution from the center outwards declines in a manner consistent with a Sersic profile.
