This galaxy appears to be a spiral galaxy viewed at a steep angle. Although there is not enough resolution to distinctly see spiral arms, there is a subtle disk shape. This morphology suggests a possible Sa or Sb classification. The color profile indicates a higher concentration of older stellar populations, with the central bulge appearing more yellow-red. This indicates ongoing, but slowly diminishing, star formation, consistent with galaxies around this mass. There is no evidence of significant tidal interactions or merging events affecting its structure. The galaxy has a smooth overall appearance, with a relatively high degree of central concentration.
