The galaxy presents an overall elliptical morphology. The core of the galaxy exhibits a concentrated, bright, yellowish-white hue. The outer regions display a gradual decrease in luminosity, fading into a more diffuse, bluish-white color. There are indications of some subtle disturbances, particularly on the periphery of the galaxy, indicating the possibility of interactions or minor mergers in the past. The overall smoothness of the light distribution suggests that the galaxy is dominated by an older stellar population, with a modest star formation rate. It has an estimated size of about 7.4 kpc. The galaxy is observed at a redshift of approximately 0.23.
