The galaxy presents as a highly elongated object, viewed nearly edge-on. A prominent central bulge is not readily apparent; instead, the light appears relatively smooth and diffuse along the major axis. There's an indication of some color variation within the disk, shifting from bluer hues towards the outer regions to yellower tones closer to the galaxy's center. The overall shape suggests a flattened disk-like structure with minimal signs of spiral arms. A slight warp or asymmetry might be present, particularly at the edges, though higher resolution data would be required to confirm. The galaxy does not appear to be undergoing a major merger or tidal disruption based on its morphology.
