The galaxy presents as a spiral type with a distinct disk structure. It exhibits two prominent spiral arms that appear loosely wound. There is evidence of a central bulge; its size appears moderate compared to the overall galactic disk. Indications of a bar structure are subtle but may be present. The galaxy's color suggests ongoing star formation, with a blueish tinge in the spiral arms. There are no clear indications of any recent major merging events, although there is the suggestion of some tidal disturbance or interaction.