The galaxy presents as a spiral galaxy, likely at a relatively small distance from our own galaxy. The spiral arms appear quite prominent, extending from a central bulge region. The bulge component looks moderate in size relative to the overall disk. The disk component appears to be the dominant feature. There is also a hint of a bar-like structure crossing the central region, though it does not stand out strongly. The overall appearance suggests it could be an intermediate spiral type. There are no signs of an active galactic nucleus or significant dust lanes are apparent in this image.
