The galaxy appears to be a relatively face-on spiral, although the arms are not well-defined and are somewhat tightly wound. The central bulge is prominent and appears nearly spherical, displaying a smooth, concentrated distribution of light. The disk component exhibits a bluer color, suggesting ongoing star formation, while the central bulge is more yellowish, indicating an older stellar population. The galaxy shows a generally smooth appearance, with only minor irregularities in its structure, suggesting minimal tidal interactions or recent merger activity. Overall, the galaxy presents as an intermediate spiral type, possibly an Sb or Sc, at an estimated distance calculated from its redshift.
