The galaxy presents as a moderately bright, elliptical morphology. Its overall light distribution appears smooth and concentrated towards the center, suggesting an older stellar population. The galaxy exhibits a centrally dominant bulge with a radial falloff in surface brightness with no distinct disk visible. The object appears fairly round in shape, with no obvious tidal features or signs of recent mergers in this image. There is some indication of weak, patchy regions of star formation, however, it is not a dominant characteristic.
