The galaxy presents a generally elliptical morphology. The light is concentrated toward the center, with a bright, compact core. The galaxy's profile appears smooth; little or no substructure, such as spiral arms or prominent dust lanes, can be discerned. There may be a faint disk structure, however it is indistinct. The galaxy has a golden-yellow hue, suggesting an older stellar population with lower levels of recent star formation. There is no evidence of tidal tails, distortions, or other signs of a major merger event. The light fades relatively smoothly with increasing radial distance from the center.
