The galaxy appears as a group of galaxies that may be gravitationally bound, as they are very close to each other. The brightest galaxy in the group appears to be an elliptical galaxy, with a smooth and diffused light profile, suggesting an older stellar population. A few other galaxies in the group appear to have disk-like features, but these features are not distinct, hinting at a less-defined spiral structure, or possible lenticular morphology. Overall, the system is relatively compact and fairly bright. There are also other galaxies nearby that might be interacting with the main group.
