The galaxy exhibits a disk-like morphology. It appears moderately inclined relative to our line of sight, preventing a clear observation of any spiral structure, but the lack of a significant bulge implies the disk makes up a large part of the visible features. There is evidence of at least one, maybe two spiral arms, though they are not well defined. The arms appear to be bluer in color, indicative of ongoing star formation. There also appears to be some amount of dust obscuring the light. The galaxy appears somewhat disturbed, possibly indicating a recent or ongoing interaction or merger.
