The observed galaxy appears to be a spiral galaxy, exhibiting a prominent, moderately sized bulge. Spiral arms are readily visible, displaying a somewhat open winding pattern. There is also a hint of a bar structure, but it appears faint. The galaxy presents a relatively high degree of symmetry with a well defined disk. The overall appearance suggests an actively star-forming galaxy, given the bluer hues along some of the spiral arm regions. There are no obvious signs of a recent major merger event, however some disturbances may be present.
