The galaxy presents as a merging system. There are what appear to be multiple distinct nuclei or bright clumps within a common, albeit disturbed, halo. The primary body of the galaxy appears somewhat elliptical, with a brighter, yellowish core suggesting an older stellar population. Extending upwards, there is a less defined, bluer region, possibly indicating ongoing star formation.

The overall structure exhibits signs of gravitational interaction. The primary nucleus appears elongated, which further indicates a disturbance. Faint tidal features might be present. The distribution of light suggests a system undergoing significant morphological transformation due to the merger event.
