The galaxy appears to be an early-type spiral, potentially exhibiting characteristics of an Sa or Sab classification. The central bulge is prominent and exhibits a yellowish hue, indicating a population of older, less massive stars. Diffuse spiral arms are present, though not sharply defined. These arms show some blueish regions, suggesting pockets of ongoing star formation, but the overall color is consistent with a passively evolving stellar population. The galaxy exhibits a relatively smooth morphology, suggesting a lack of recent major mergers or significant interactions. Faint tidal features cannot be completely ruled out based on this image alone. The galaxy's disk appears somewhat inclined relative to our line of sight.
