The observed galaxy presents as a merging system, exhibiting two primary components. The larger of the two galaxies appears generally smooth and elliptical, with a concentrated, bright core, and a diffuse halo. The color is generally redder, suggesting an older stellar population and suppressed star formation. The smaller galaxy is located nearby, but appears to be more compact and less diffuse than the larger one. It has a distinct yellow core. There's a faint bridge of material connecting the two galaxies, suggestive of tidal interactions and ongoing merger activity. Overall, the galaxy system appears to be in a late stage of merging, with potential ongoing star formation in the merging core.
