This galaxy presents a complex morphology, suggestive of a system undergoing a significant interaction, possibly a merger. The dominant light profile suggests a generally smooth appearance overall, with some disturbed features.

There are two distinct luminosity peaks, one with a bluer spectral component and the other with a redder spectral component. The system exhibits moderate overall roundness, and there is little evidence of tidal tails or other strong indicators of recent major mergers. While appearing generally smooth, closer inspection reveals asymmetry indicative of gravitational disturbances from a merger event. The colors suggest moderate active star formation.
