The galaxy presents a disk-like morphology, although the angle of observation is such that it is significantly inclined, nearing an edge-on perspective. The central bulge appears relatively small in comparison to the overall galactic disk size. Spiral arm structures are subtly visible, appearing somewhat tightly wound. A slight asymmetry is observed, possibly indicative of a minor interaction or disturbance. The overall color suggests a mix of stellar populations, with a yellowish central region likely indicative of older stars, and bluer hues in the disk hinting at ongoing star formation. There does not seem to be a central bar. The disk appears smooth.
