The galaxy presents as a system with multiple components and apparent disturbances, suggestive of an ongoing or recent interaction. It exhibits a moderately smooth overall appearance, however a faint disk-like structure is present.

The primary body of the galaxy is elliptical with an apparent major axis of approximately 10,000 parsecs. The color gradients suggest a modest population of younger stars. A secondary, smaller component shows bluer hues, indicative of more active star formation. This secondary component is offset from the center of the main body.

Evidence of tidal disruption is present in the form of faint extensions or plumes emanating from the primary body. These structures are subtle, but suggest a gravitational interaction with another galaxy.
