The galaxy appears to be an elliptical galaxy, showing a smooth, featureless morphology. It has a central concentration of light, suggesting an older stellar population. The color gradient indicates it is redder in the center and becomes slightly bluer moving outward, implying the possibility of more recent star formation towards the galaxy's periphery, although this is more likely due to noise. The shape seems mostly round with a hint of elongation along one axis. There is no evidence of spiral arms, dust lanes, or other prominent structures typically associated with spiral or irregular galaxies, and no apparent mergers, though there may be some slight tidal disturbances.
