The galaxy presents a complex morphological structure, appearing to be in the midst of a significant interaction or merger. A dominant, relatively smooth and luminous component exhibits a yellowish hue, suggesting a population of older stars. This core region is somewhat elongated in shape, not perfectly spherical.

Extending from this core, there is a more diffuse and less luminous component, appearing slightly bluer in color, potentially indicating ongoing or recent star formation. This feature is irregular and distorted, suggestive of tidal interactions. The overall structure is disturbed and asymmetric, lacking a clear spiral arm structure or well-defined disk. The interaction or merger seems to be disrupting the galaxy's original morphology.
