The galaxy appears to be a relatively bright object with a notable central bulge. The overall color profile suggests a mixture of stellar populations, with the core exhibiting a yellowish-white hue indicative of older, more evolved stars. Fainter, bluer regions suggest the presence of some younger stars and potential star formation, although these regions are not particularly pronounced.

The galaxy's morphology is somewhat disturbed, with hints of tidal features or irregular extensions that might indicate past interactions or mergers. There appear to be asymmetries in the outer regions of the galaxy's disk. The overall structure indicates a transitionary stage between a spiral galaxy and a more amorphous form, possibly an elliptical galaxy.
