The galaxy exhibits a prominent disk structure, viewed at an angle that is nearly face-on. The spiral arms are well-defined, displaying a two-armed morphology. The winding of the spiral arms appears to be moderate. The central bulge of the galaxy appears moderate in size. A weak bar structure is possibly present within the central region. The galaxy does not appear to be undergoing any major merging events or significant tidal disturbances. There appears to be some evidence of current star formation.
