The galaxy presents as a spiral galaxy, viewed at an angle that is not quite edge-on, but not fully face-on either. The spiral arms are moderately defined, with a flocculent structure. Areas within the arms exhibit clumpy regions, suggesting zones of active star formation. The central bulge appears relatively small, with an indistinct shape. The galaxy does not appear to have any prominent bar structure. There are no signs of strong tidal disturbances or interactions with other galaxies. The galaxy is resolved well enough to observe some of the underlying structure but not in great detail, meaning its distance is likely intermediate. Overall, this spiral galaxy seems to be in a relatively undisturbed state of evolution.
