The galaxy appears to be a disk galaxy, viewed at a moderately oblique angle. It exhibits a prominent central bulge that appears relatively smooth and bright. The disk component is visible, though somewhat indistinct, showing evidence of spiral structure. The color profile suggests a moderate level of star formation, with some blue hues indicating the presence of younger stars. There is a slight indication of dust lanes within the disk, obscuring some of the starlight. The overall shape is somewhat rounded, although there is a slight elongation along one axis. There appears to be no indication of a major merger in progress, however, there may be some minor disturbance within the spiral arms.
