The galaxy presents as a moderately luminous object, exhibiting a generally smooth morphology. Its overall shape is elliptical, appearing largely round but with a hint of elongation. There is some visual evidence of a minor disturbance or interaction. A neighboring component exists, with a separation that suggests an ongoing or recent merging event. The galaxy's color indices indicate a population dominated by older stars. The relatively low star formation rate is consistent with a massive galaxy that is nearing quiescence. The estimated mass points to a large galaxy.
