The galaxy presents as a merging system. There appear to be two distinct nuclei visible, one brighter than the other. The brighter nucleus exhibits a yellow-white hue, suggestive of an older stellar population. The fainter nucleus, positioned to the lower right of the brighter nucleus, exhibits a similar color profile.

A diffuse halo surrounds both nuclei, indicating possible tidal interactions. The shape of the halo appears to be elongated, further supporting the merging scenario. Faint bluish extensions are seen emerging from the halo, possibly indicating regions of ongoing star formation triggered by the merger event. The overall morphology deviates significantly from a regular elliptical or spiral shape. This is most likely the result of gravitational disturbances related to the ongoing merger event. The overall color profile leans towards a redder spectrum indicating an older stellar population. There are also features indicative of dust absorption occurring around the nuclei, though these observations are faint.
