This galaxy appears to be a relatively smooth, elliptical type galaxy at a redshift of approximately 0.19. The light distribution is centrally concentrated, indicating a significant bulge component. The galaxy exhibits a generally rounded morphology. There appears to be a possible minor disturbance or tidal feature. The light profile suggests an older stellar population, which is supported by the redder colors of the galaxy's bulge. The blue light might suggest some recent star formation. Overall, it appears to be a fairly massive galaxy with ongoing, but moderate, star formation.
