The galaxy appears to be a spiral galaxy viewed at a moderate inclination. The central bulge is moderately prominent and shows a smooth texture, possibly indicating an older stellar population. Spiral arms are visible, but somewhat faint and not clearly defined, suggesting they might be loosely wound. There is some indication of disturbance, possibly caused by a past interaction or merger. This is subtly indicated by slight asymmetry in the distribution of the galactic disk's light. The color gradient suggests active star formation may be present, especially within the disk, giving it a slightly bluer hue compared to the central region, which appears more yellowish. Overall, this galaxy presents features of both smooth structure and mild disturbances within the spiral disk.
