This galaxy presents as a moderately luminous, elliptical structure at a redshift of approximately 0.18. It exhibits a centrally concentrated bulge with a relatively smooth light distribution. There's a subtle indication of a disk component. The galaxy is neither perfectly spherical nor significantly elongated, exhibiting an intermediate shape, with a strong central yellowing. No major merger events are apparent and no significant tidal disturbances or debris tails are discernible, although there could be minor disturbances. Its stellar mass is significant, approximately 10^11 solar masses, while its star formation rate is relatively low, implying a quiescent state. The overall color suggests a population dominated by older stars.
