This galaxy appears to be in a state of interaction or merger with another galactic object. There is a primary, somewhat amorphous core of moderate luminosity and color temperature consistent with a mature stellar population. Connected to this core is a tidal bridge or tail-like structure, slightly fainter but of similar color. At the other end of this structure is what appears to be a second concentration of stellar density, indicating a possible secondary nucleus or a significant tidal dwarf galaxy formed during the interaction. The overall morphology is highly disturbed and deviates significantly from a regular elliptical or spiral form. The system exhibits moderate estimated mass and ongoing star formation based on photometric data.
