The galaxy appears to be undergoing a significant merger event. Multiple distinct nuclei are visible within a disturbed, diffuse halo of light. The galaxy is overall fairly round with no defined spiral arms. The color of the galaxy is yellowish-orange, indicating a likely older stellar population and suppressed star formation within the merging system. There is evidence of ongoing tidal interactions, evidenced by the disturbed morphology. The overall luminosity of the galaxy is high.
