The galaxy presents as a spiral galaxy, likely of type Sb or Sc. The spiral arms are clearly present, though somewhat tightly wound, exhibiting a relatively high degree of symmetry. The central bulge is moderately sized and exhibits a more pronounced luminosity and yellowish hue, indicating a greater concentration of older stellar populations. The disk component shows bluer patches, likely indicative of younger, hotter stars within star-forming regions along the spiral arms. The overall morphology suggests that the galaxy is relatively undisturbed, with no obvious signs of a recent major merger event. The disk appears almost face-on, with only a slight inclination to our line of sight. There is evidence of a bar structure, but it is not exceptionally strong, indicating a moderately barred spiral morphology.
