The galaxy presents as a flattened, disk-like structure, viewed at a noticeable angle that suggests it is not quite edge-on but not quite face-on either. Its central region exhibits a high degree of smoothness, indicating an elliptical component or a bulge in the disk. The light intensity is concentrated towards the center, forming a bright, yellowish core, suggesting an older stellar population and potentially low levels of current star formation within this area.

Moving outward from the core, a faint, bluer disk is observed, which contributes to the overall disk-like morphology. The disk appears relatively smooth with little to no spiral arm structure that can be discerned at this resolution. Some minor irregularities or disturbances are present, with a slight asymmetry in the outer regions of the galaxy, hinting at a possible past interaction or minor merger event. The overall color gradient shifts towards the blue at the edges, which implies a younger, actively star-forming population in the outer regions compared to the core.
