The galaxy presents as a relatively smooth, centrally concentrated object with an elliptical morphology. It exhibits a bright, yellowish core that gradually fades into a less defined outer region. There are subtle color variations within the galaxy, with a hint of redder hues in the outer regions compared to the more yellowish central bulge. No distinct spiral arms or features are readily apparent. The overall structure appears undisturbed, with minimal signs of ongoing or recent merger activity. The galaxy appears to have a moderate degree of roundness, not extremely spherical but also not highly elongated. The estimated redshift suggests a significant distance, meaning we are observing the galaxy as it was some time ago. Star formation appears to be relatively low.
