The galaxy presents an elliptical morphology, exhibiting a smooth, concentrated central bulge. The luminosity appears to be fairly evenly distributed with a slight flattening towards a cigar shape. Evidence for spiral arms is not apparent.  There are subtle color variations suggesting a change in stellar populations from the core to the outer regions, with the core exhibiting a more yellow/orange hue compared to the blue halo. The galaxy does not appear to be undergoing any major merging events, though there are possibly some minor distortions in the outer regions of the galaxy that could indicate minor interactions or disturbances. 
