The galaxy appears to be an elliptical galaxy at a redshift of approximately 0.13. The galaxy exhibits a generally smooth morphology, with a high degree of central concentration. There is no apparent spiral structure or significant disk component visible. The color is generally redder, with a slightly yellowish core and gradually fading redder halo. There are no indications of ongoing major mergers or significant tidal disturbances; any disturbances are at a minor level. The object's roundness indicates that it is not highly elongated, and is considered well-rounded. Overall, the galaxy likely consists primarily of older stellar populations, with a low rate of star formation.
