The galaxy appears as a small, relatively faint, and somewhat elongated object. It exhibits a smooth, featureless morphology, suggesting a lack of prominent spiral arms or irregular structures. The light distribution appears concentrated towards the center, with a gradual decrease in brightness towards the outer edges. The galaxy displays a yellowish-white hue, indicative of an older stellar population with a reduced rate of ongoing star formation. The overall appearance is consistent with an elliptical or lenticular galaxy at a moderate cosmological distance, approximately 560 megaparsecs. There is no visual evidence of significant tidal disturbances or interactions with neighboring galaxies.
