The galaxy exhibits a moderately inclined disk-like structure. A prominent central bulge dominates the overall light profile, appearing smooth and concentrated. Faint spiral arms extend from the central bulge, showing relatively open morphology with moderate disturbances to the disk shape. These arms appear to be bluer in color than the bulge. There is no indication of ongoing major merging activity; however, minor disturbances appear present. The galaxy does not appear to have a strong bar structure. The galaxy's disk is not observed perfectly edge-on, and has a slight inclination towards our line of sight.
