The galaxy presents an edge-on disk morphology. It exhibits a prominent central bulge, which appears rounded and dominates the overall luminosity. The disk component is relatively smooth, with no readily discernible spiral arm structure. The color gradient indicates a redder bulge compared to the slightly bluer disk. There is no clear evidence of ongoing major merger activity, though a minor disturbance cannot be ruled out. The overall light distribution suggests a relatively quiescent system with a moderate stellar mass.
