The galaxy appears to be a spiral galaxy observed at an oblique angle. There is a noticeable bulge, appearing yellowish-orange, concentrated towards the center. The spiral arms extending from the bulge are faint and somewhat indistinct. There is also a blueish tinge on one side of the galaxy, which might indicate active star formation, but it is too faint to determine for certain. The morphology suggests there may be a minor disturbance in the galaxy's overall structure, though no major merger events are observed. The overall structure seems relatively undisturbed. The galaxy presents a moderate level of star formation and a relatively high mass.
