The galaxy presents as a relatively smooth, disk-like structure, exhibiting a flattened, elongated shape indicative of a spiral or lenticular type galaxy. There is little evidence of a prominent central bulge, although some increased light concentration is visible in the center. Color gradients are subtle, with a somewhat bluer hue, this suggests ongoing star formation within the galaxy. There are subtle hints of spiral arm structures, though not well-defined, indicating a possibly disturbed or flocculent spiral pattern. There is little evidence of recent or ongoing major merger activity, though a small amount of disturbance is possible.
