The galaxy appears to be a relatively compact object with a bright, concentrated central region. The light profile suggests a degree of central concentration that may indicate a supermassive black hole at the center of the galaxy. The color distribution within the galaxy appears somewhat complex. The inner region displays a bluer hue, which could be indicative of younger stars or a higher rate of star formation. The presence of a few outer patches of less concentrated light suggest there may be some recent or ongoing disturbance. There does not appear to be any spiral arm structure, and there also isn't evidence of a bulge, although these features may be too faint to resolve clearly in this image.
