The galaxy presents as a somewhat elliptical structure, with a concentrated central bulge that emits significantly more light than the outer regions. This bulge appears a yellowish-white hue, suggesting an older stellar population. The light from the rest of the galaxy fades from the yellowish-white central bulge to a blueish tint that forms a disk. The image suggests a fairly smooth light distribution overall, without prominent spiral arm structures that are commonly found in spiral galaxies. There is little indication of ongoing major star formation based on this image.
