The galaxy presents an overall ellipsoidal morphology, appearing somewhat elongated. It exhibits a prominent central bulge, characterized by a high concentration of light, indicating a significant population of older stars. The bulge displays a yellow-orange hue. Moving outwards from the central region, there appears to be a fainter disk component, possibly with some faint spiral arm structure or irregularities, though its organization is not clearly defined. The disk component is bluer in color than the bulge. There may be a faint tidal feature suggesting possible past interaction or a minor disturbance, but overall it doesn't present as a late-stage merger.
