The galaxy presents as a flattened, elliptical structure with a distinct central bulge. The bulge exhibits a concentrated, yellowish-white hue, suggesting a population of older, evolved stars. Moving outward from the core, the galaxy displays a less concentrated, somewhat bluer disk. The disk appears relatively smooth, with only subtle indications of spiral arm structures. There is evidence of ongoing star formation as indicated by a light blue hue in the outer regions of the disk. Overall, the galaxy exhibits characteristics intermediate between a pure elliptical and a spiral galaxy, showing features of both morphological types. There may be some tidal distortion visible, as there appear to be disturbances in the disk.
