Observed is a likely merging or interacting system. The primary object appears as a relatively smooth, roundish form, but with an apparent second component, potentially a merging galaxy, creating a binary appearance. Definite disturbance is occurring, as the color appears to be changing. A small fraction of the mass also has a very bright blue tint. This galaxy has an angular size just above that of a point source at this level of observation. The system shows a distinct color gradient, shifting from redder hues within the primary central region to bluer tones toward the outer regions, indicating active star formation. The overall structure seems to be in a state of flux, with significant tidal interactions likely influencing the observed morphology.
