The galaxy presents as a merging system, with a primary, spheroidal component and a smaller, seemingly disrupted secondary component. The primary galaxy exhibits a smooth, elliptical morphology with a concentrated, yellowish core, suggesting an older stellar population. Its overall shape appears roughly round. The secondary component, located to the south, displays a bluer hue with a less defined structure, potentially indicating ongoing or recent star formation activity and younger stars. A significant portion of the overall light appears to be concentrated in the merging or interacting region between the two components. There is evidence of tidal disturbances or asymmetries suggesting possible strong gravitational interactions between the two galaxies, and the system is likely in an advanced state of merging based on the disturbed morphology. Overall, the system appears to be a dynamically evolving structure.
