The galaxy presents as a merging system, with what appears to be two primary galactic nuclei. The morphology indicates an ongoing interaction, possibly a later stage merger given the apparent proximity of the two galactic cores. There is evidence of tidal disruption around the central regions, with a slightly extended but diffuse outer halo exhibiting a yellowish color profile. The primary galaxy has a more rounded morphology, while the second galaxy appears more elliptical in shape, suggesting the initial progenitors may have been an elliptical and a spiral galaxy, respectively. Overall, the system's structure is complex, with an apparent central overdensity of older stellar populations. The estimated size suggests a relatively massive system. The color profile appears generally red-shifted across the galaxy, consistent with a more passive star formation rate in the galaxy.
