The galaxy appears to be a smooth, elliptical-like structure with a generally round morphology. Its light is a yellowish orange hue. It appears to be composed of primarily older stars. There is no distinct nucleus visible, and there are no obvious spiral arms or prominent dust lanes present. It appears undisturbed with no significant signs of tidal interactions or recent mergers. However, there are some irregular aspects to the galaxy, suggesting there is a high chance that it has merged with another galaxy in the past. There appear to be multiple regions of more intense light. This could be a galaxy undergoing the process of merging.
