The galaxy appears to be an interacting or merging system, exhibiting significant tidal disruption. The primary body presents as a smooth, elliptical structure with a yellowish-gold hue, suggesting an older stellar population and relatively low levels of ongoing star formation. There is evidence of a smaller, secondary component, possibly another galaxy in the process of merging. This component is somewhat bluer in color, indicating some more recent star formation. Debris are scattered throughout the galaxy system with at least two very bright regions of interaction. The galaxy is slightly elongated, hinting at either a disk component viewed at an angle or the ongoing gravitational distortion from the interaction. Overall, the galaxy seems to be relatively massive, based on its size and the luminosity of its stellar population.
