The galaxy presents as a spiral type, exhibiting prominent, loosely wound spiral arms. These arms emanate from a central bulge region, which appears moderately sized relative to the overall disk. There is evidence of a bar structure within the central region, though its definition is somewhat weak. Patches of bluer light, indicative of active star formation, are scattered throughout the spiral arms. The disk appears somewhat disturbed on one side of the galaxy. The galaxy is inclined at an angle relative to our line of sight, allowing a partial view of its disk structure.
