The galaxy presents as a somewhat amorphous, centrally concentrated structure. A faint disk component may be present and oriented diagonally across the image frame, however, its structure is irregular. There is evidence of a possible tidal tail extending from the main body of the galaxy, suggesting past or ongoing gravitational interactions with another galaxy, or perhaps an ongoing merger event. The galaxy exhibits a pale yellowish-white hue, indicating an older stellar population with moderate amounts of on-going star formation. The system's overall roundness suggests a classification somewhere between a spiral and an elliptical galaxy, but the potential tidal feature implies it is disturbed.
