The galaxy presents as a single, relatively smooth object with a concentrated central region. Its morphology is elliptical in nature, exhibiting a high degree of roundness. The color distribution suggests a dominant population of older stars, evident in the yellowish-red hue of the main body. There is also some evidence of what appears to be bluer emissions on the edges of the galaxy, though they are fairly dim and hard to make out. We are seeing the galaxy at a time when it is undergoing very little star formation.
