The galaxy presents as an elongated, disk-like structure, viewed at a moderate angle, suggesting it is neither perfectly edge-on nor face-on. The central region appears brighter and more diffuse, potentially indicating the presence of a galactic bulge. A notable feature is the asymmetrical distribution of light, with one end displaying a distinct, reddish-orange hue. This could indicate a region of active star formation or dust obscuration. The overall morphology displays some signs of disturbance, possibly due to interactions with other galaxies. There may be some ongoing minor mergers. The remaining portions of the galactic disk are characterized by a bluer color, possibly indicating younger stellar populations.
