The galaxy presents as a merging system, exhibiting a clear interaction between two distinct galactic components. The larger component displays a predominantly smooth morphology, with a centrally concentrated, bright core emitting strongly in the redder wavelengths. This suggests an older stellar population dominating its composition. Evident tidal features indicate gravitational disturbances. 

A second, smaller component, is visibly separate, located at a short distance from the primary galaxy. It exhibits a less defined morphology compared to the larger component, appearing somewhat diffuse. The color profile suggests a less prominent presence of younger, bluer stars relative to the larger component, but this could be an observational effect.

There is evidence of ongoing interaction between the two galaxies. It appears that the smaller component is in the process of merging with the larger galaxy.
