The galaxy appears to be a system of two interacting galaxies at an estimated distance. The primary galaxy exhibits a smooth, elliptical morphology. It displays a concentrated, bright core with a diffuse, extended halo. The overall color is indicative of an older stellar population.

A secondary galaxy is positioned some distance from the primary galaxy. This component appears to have a more irregular shape. There is an indication of tidal distortions, suggesting gravitational interaction between the two galaxies. The secondary galaxy also has a significant component of an older stellar population.

There appears to be a stream of material between the two galaxies, but this may be an artifact.
