The observed galaxy appears to be undergoing a merger or strong tidal interaction. A primary, relatively smooth and compact component is visible. This primary component exhibits a somewhat rounded morphology. 

Connected to the primary galaxy is a more diffuse region, suggesting a significant tidal disturbance. The color in this region shifts towards the blue end of the spectrum, suggestive of active star formation within the disrupted material. The blue color and diffuse morphology contrast with the yellowish core of the main body.

 There may be some evidence of a faint tidal tail or extended feature emanating from the merging system. Overall, this galaxy is a dynamic system characterized by morphological disturbance, potential tidal features, and varying stellar populations indicative of an ongoing interaction.
