The galaxy presents a somewhat amorphous morphology, with a blue-ish hue dominating its central and peripheral regions. There is a subtle, diffuse, extended disk-like structure. The galaxy does not display a prominent central bulge; instead, the light distribution appears fairly uniform across the visible extent of the galaxy. Faint hints of possible spiral arms can be seen, but the overall structure is more akin to a flocculent spiral or an irregular morphology. There's indication of active star formation, with regions of bluer light suggesting the presence of young, hot stars. There are some hints of a disturbance in the morphology of the galaxy, possibly indicating minor merging events.
