The galaxy presents as an elliptical or lenticular type with a relatively smooth appearance. Its color profile indicates a predominantly older stellar population with a yellowish-orange hue suggesting a paucity of recent star formation. The morphology suggests a centrally concentrated light distribution, with the luminosity gradually decreasing towards the outer regions. There is no indication of prominent spiral arms or a well-defined disk structure, suggesting a dynamically relaxed system. The galaxy exhibits a moderate redshift, which places it at a substantial cosmological distance. Overall, the visual characteristics are consistent with a massive, early-type galaxy that has largely ceased significant star formation activity.
