The galaxy presents as a centrally concentrated, somewhat rounded structure. The core exhibits a bright, yellowish-orange hue, suggesting an older stellar population and/or significant dust obscuration. A faint, greenish halo surrounds the core. This suggests ongoing, albeit possibly subdued, star formation within the outer regions. No distinct spiral arms or bar features are discernible at this resolution. The overall morphology appears relatively smooth, lacking evidence of major tidal disturbances or ongoing merger activity. The galaxy exhibits a redshift indicating a significant distance. Considering these features, the galaxy appears to be an elliptical or lenticular type galaxy, possibly undergoing only minor star formation in its outer regions.
