The galaxy presents as a moderately luminous object at a redshift of approximately 0.08, indicating a considerable distance. It exhibits a generally smooth morphology, with a slight elongation of the central structure. A faint disk component is potentially discernible, but not definitively. The light distribution suggests an elliptical galaxy. The colour indices suggest a moderately evolved stellar population, with no intense bursts of recent star formation. Indications are that the central bulge is a significant component of the overall morphology, which is largely undisturbed.
