The galaxy presents as a slightly elongated structure, though approaching a circular form. A hint of spiral structure is visible, yet the arms are not sharply defined. The core exhibits a bright, concentrated center that gradually fades outwards. The light distribution suggests a relatively smooth transition from the nucleus to the outer regions, indicating a galaxy somewhere between a pure elliptical and a spiral. There are hints of subtle disturbances in the outer regions, suggesting possible past interactions, though these are not pronounced enough to suggest an ongoing major merger event. The overall color is slightly reddish, with some bluer star-forming regions mixed in, suggesting that this is a reasonably massive galaxy with moderate star formation activity, and that it could contain an older stellar population.
