This galaxy exhibits characteristics of a spiral galaxy, though its structure appears somewhat disturbed. A central bulge is visible, exhibiting a yellow-white color, suggesting an older stellar population. Fainter, diffuse spiral arms extend outwards, displaying a bluer hue indicative of ongoing star formation. The morphology of the arms appears irregular, showing signs of possible tidal interactions or past minor mergers. The light distribution indicates a luminous galaxy. Overall, the galaxy appears to be undergoing relatively modest star formation. Evidence indicates potential minor disturbances in its structure possibly related to galactic merging events.
