The galaxy presents as a moderately luminous object with a redshift of approximately 0.37. It exhibits a somewhat elliptical morphology, appearing predominantly smooth with a subtle disc-like structure. The galaxy's color suggests a significant population of older stars, indicating a relatively low star formation rate. There is evidence of a potential minor disturbance in the morphology, perhaps suggesting a past interaction or minor merger event. The light distribution is centrally concentrated, indicative of a substantial central mass. Overall, this galaxy appears to be a relatively massive and evolved system.
