The galaxy presents as a complex structure, potentially undergoing an interaction or merger. A dominant, relatively smooth and featureless, central component exhibits a somewhat elongated profile. The light distribution suggests a concentration of older stars.

Connected to this central mass is a fainter, less defined structure. This component shows some indication of bluer colors, potentially indicative of ongoing or recent star formation. The morphology could suggest tidal features resulting from an interaction, although a definitive classification is hindered by the image resolution. The system as a whole does not appear perfectly symmetrical, further supporting the possibility of external influence on its structure.

Overall, this galaxy presents an interesting case for further study to fully characterize its dynamics and evolutionary history.
