The galaxy presents as a merging system, characterized by two distinct, luminous components suggestive of galactic nuclei in close proximity. A diffuse, lower-surface-brightness envelope surrounds the nuclei, indicating tidal interactions and disturbed morphology. The system appears relatively smooth, with no clearly defined spiral arm structures visible within the resolution of the image. The color is predominantly yellowish. The apparent angular size is small. Overall, the galaxy shows strong evidence of ongoing or recent merger activity.
