The galaxy presents as a centrally concentrated object, exhibiting a predominantly smooth morphology. The light distribution suggests a spheroidal shape, with a gradual decrease in intensity from the core outwards. The color profile indicates a redder core region transitioning to slightly bluer outer regions. There is no apparent spiral arm structure or significant dust lane obscuration visible at this resolution. A slight asymmetry is observed in the outermost regions, possibly indicating minor tidal disturbances or interaction with smaller companions. Overall, the galaxy appears to be an elliptical or lenticular type with no major ongoing merger activity.
