The galaxy presents as a spiral type, viewed at an oblique angle. A moderate bulge is visible at the center, exhibiting a bright core. From the core, spiral arms extend outwards; these arms appear tightly wound. These arms are not uniform, showing variations in luminosity and color, suggesting differing stellar populations and dust distributions. The majority of the arms appear to contain active star forming regions, indicated by their bluer tint. There is a possible weak bar structure bisecting the central bulge. The overall morphology suggests the possibility of a minor gravitational disturbance, as the spiral arms show some signs of asymmetry. It's spiral arms are mostly observed to have between 1 and 4 arms.
