The galaxy exhibits a flattened, elliptical morphology, with a distinct bulge and a disk oriented at an angle to our line of sight. The central region appears brighter and more concentrated, suggesting a higher density of stars. Moving outward from the core, the luminosity decreases gradually. The disk shows hints of a spiral structure, with subtle color variations that may indicate differences in stellar populations and dust distribution. Overall, it exhibits properties consistent with a late-type spiral galaxy, possibly transitioning towards an elliptical morphology due to ongoing or past interactions.
