The galaxy presents as an elliptical system with evidence of a recent or ongoing merger event. It exhibits a relatively smooth overall structure with a high degree of central concentration. The galaxy's shape appears somewhat elongated, deviating from a perfectly circular morphology. There is a distinct redder, roundish concentration of light slightly offset from the main body and the main body has a more yellowish appearance. The system does not display any prominent spiral arm structures or a well-defined disk component. The presence of an apparent disruption and the redder separate concentration of light are consistent with characteristics often observed in galaxies undergoing mergers. There are some indications that significant star formation may be suppressed overall, as the bluer light, which would suggest more recent star formation, is diminished.
