The galaxy appears to be a spiral type, oriented roughly face-on relative to our line of sight. It exhibits a prominent central bulge, which appears yellowish-white in color, suggesting an older stellar population. The disk is relatively well-defined, displaying faint spiral arm structures. Two main arms are discernible, appearing somewhat tightly wound around the bulge. There is evidence of bluer regions within the arms, indicative of ongoing star formation. The galaxy displays a moderate bar structure extending through its center. There may be evidence of a minor disturbance in the disk morphology, however there are no strong indicators of an ongoing major merger. The overall light distribution indicates a moderate size, with a notable bulge component and active star formation regions within its spiral arms.
