The galaxy presents as a likely merger event, involving at least two distinct galactic nuclei, exhibiting a yellow-orange hue. The morphology suggests a relatively evolved system, potentially an elliptical galaxy in formation. The overall shape is somewhat irregular, indicative of gravitational interactions and tidal forces between the merging components. There may be regions of elevated star formation, indicated by the slight bluer tones in certain areas, however it appears quite low overall. The system is relatively compact and smooth, lacking prominent spiral arms or well-defined disk structures. The merging process appears to be in its later stages, with significant overlap between the two galaxies. There is a faint tidal tail or stream extending from one side of the primary galaxy.
