This galaxy appears as a centrally concentrated object with a smooth morphology. There is a gradual decrease in luminosity from the bright, seemingly spherical core to the outer regions of the galaxy. The galaxy's color profile suggests the presence of a relatively older stellar population with potentially ongoing star formation. I see minimal evidence of spiral arm structures, which leads me to believe that it is likely an elliptical or lenticular galaxy, although some disk features may exist. There is some distortion in shape which could indicate a minor disturbance happening with a merger.
