The galaxy presents as a somewhat irregular disk galaxy, exhibiting features that suggest possible interactions or disturbances. It is not observed perfectly face-on, as the disk appears slightly tilted relative to the line of sight. The galaxy displays spiral arm structure that seems loose and ill-defined. Star formation is present, as indicated by regions exhibiting a blue hue. A central bulge is not evident, or if it exists, is very small. The galaxy appears to be undergoing an interaction or a merging event that could involve minor or major disturbance of its structure, with the galaxy's morphology displaying hints of these potential disturbances. It is actively forming stars at a low rate.
