The galaxy presents as an elongated, disk-like structure with a notably high degree of axial symmetry. Its color profile suggests a prominent, central bulge region characterized by a reddish-orange hue, potentially indicating an older stellar population and reduced levels of ongoing star formation within this area. The outer regions of the galaxy display a bluer tint, possibly indicative of younger stars and more active star-forming regions in the galaxy's spiral arms. Overall, the galaxy's morphology is consistent with that of a spiral galaxy viewed at an oblique angle, close to edge-on. There appears to be a lack of any strong tidal features or morphological distortions, suggesting it is relatively undisturbed and has not experienced any recent major merger events.