The galaxy presents an extended morphology with a noticeable disk-like structure, although the disk is not sharply defined. The color gradients suggest active star formation regions, with a dominant greenish hue that indicates ionized gas emission, possibly from HII regions within the disk. There may be low level disturbances in the overall morphology. It is hard to discern the exact origin of such disturbances. The galaxy appears relatively diffuse. The galaxy exhibits a level of structural complexity that might imply past interactions.

