The galaxy presents as an elongated structure, likely a disk galaxy viewed at a high inclination. A concentrated central bulge is evident, appearing relatively smooth and bright. The outer regions of the galaxy appear more diffuse and less defined, suggesting a fading stellar population or a gradual decrease in star formation activity away from the galactic center. There might be some dust obscuration throughout. The overall color appears somewhat redder, suggesting an older stellar population and/or the presence of dust within the galaxy. No strong spiral arm structure is immediately apparent. There are likely few signs of any major ongoing merger events or significant tidal disturbances.
