The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. A dominant, bright core is observed, surrounded by a more diffuse halo of light, which fades gradually into the background sky. The light from the galaxy appears to be composed of a yellow/orange color gradient, which is concentrated at the core, indicating a population of older stars. There appears to be a small redder region off to the right of the galaxy, possibly an area of ongoing star formation. There is no evidence of spiral arms or a significant disk structure.
