The galaxy presents as a disk galaxy, viewed at an oblique angle, but not quite edge-on. The central bulge appears prominent and is yellowish-white in color, suggesting an older stellar population. The disk itself shows a bluer hue compared to the bulge, indicative of ongoing or recent star formation. There is some evidence of spiral arm structure, though it appears somewhat flocculent and not tightly wound. The galaxy's overall shape suggests a well-defined disk, but with some degree of internal disturbances or asymmetries. The light distribution fades gradually towards the edges of the disk.
