This galaxy appears to be an elliptical galaxy at a redshift of approximately 0.158, indicating a significant distance. It exhibits a largely smooth morphology, with a high degree of central concentration. The galaxy has a generally round shape. There is no evidence of significant ongoing merging activity or major disturbances in the galaxy's structure, though minor disturbance is possible. Based on its color and estimated absolute magnitudes, this galaxy likely consists of an older stellar population, with a relatively low rate of star formation.
