The galaxy presents as a moderately inclined spiral, with a relatively bright central bulge. The disk component is readily apparent, showing some structure suggestive of loosely wound spiral arms. A notable feature is a prominent central bar structure that seems to dominate the inner region, adding to the overall luminosity there. The outer regions of the disk fade in intensity. Overall, it appears as a spiral galaxy with a prominent bar, with the disk exhibiting signs of ongoing star formation.
