The galaxy presents as an elliptical system at a redshift of approximately 0.137, indicating a significant distance. The galaxy's light profile appears smooth and centrally concentrated with a high degree of roundness in its overall shape. The core region exhibits a bright, yellowish-white hue, suggesting a concentration of older stellar populations. The galaxy lacks any pronounced spiral arm structure or significant dust lanes, further supporting its classification as an elliptical galaxy. There is a subtle colour gradient with the outer regions appearing slightly redder, potentially indicative of older, cooler stars. The lack of any distinct morphological disturbances suggests it is a relatively isolated system that isn't undergoing any major merging events, although minor tidal interactions can not be ruled out. Based on the colour and morphology, this galaxy is likely to have a high stellar mass and a low rate of star formation.
