This galaxy appears to be a spiral galaxy at a considerable distance, with a redshift of approximately 0.25. The overall morphology suggests a disk galaxy, although the arms are not sharply defined.

The central region of the galaxy exhibits a yellow-ish hue, possibly indicating an older stellar population with lower levels of ongoing star formation in the galactic bulge. Moving outward from the center, the disk shows some patchy blue regions, hinting at younger, hotter stars and active star formation.

There are no clear signs of a major ongoing merger event, though a slight asymmetry or disturbance in the disk could indicate past interactions or minor mergers. The galaxy's structure appears somewhat irregular or flocculent, rather than a grand design spiral, suggesting ongoing gravitational interactions or internal dynamical processes.
