The galaxy appears to exhibit characteristics consistent with a merging system or a galaxy undergoing significant tidal disruption. It displays a complex morphology with a notable asymmetry in its structure. The primary body appears to be composed of a central, yellowish core, which suggests an older stellar population. Adjacent to this core, there is a distinct, more diffuse bluish component, possibly indicative of recent star formation activity. This juxtaposition of color suggests spatial segregation of stellar populations within the galaxy. A tail-like feature or extension appears emanating from the main body. The light distribution is not uniform, indicating potential ongoing gravitational interactions or internal disturbances that are influencing the galaxy's overall structure. The edges of the structure appear fuzzy and undefined indicating ongoing interactions.
