The galaxy presents as a spiral, exhibiting a disk-dominated morphology. Two prominent spiral arms are observed with a loose winding pattern. The central bulge appears small to moderate in size, with no readily apparent bar structure. There is a distinct color gradient observed, with a yellowish central region, potentially indicating an older stellar population, transitioning to bluer hues in the spiral arms, suggestive of ongoing star formation. There appear to be major disturbances or merging events occurring in the galaxy, likely contributing to its irregular spiral arm structure.
