The galaxy presents as an elliptical or lenticular system at a redshift indicating an appreciable distance. Its morphology is dominated by a smooth, featureless light distribution, with a highly concentrated core. The galaxy exhibits a rounded shape, with a very slight deviation towards elongation but approximates a circular form in projection. The overall color appears relatively uniform across the galaxy, trending towards a redder hue, indicative of a stellar population dominated by older, redder stars and suggesting relatively low on-going star formation. There is little evidence of spiral arms, dust lanes, or other distinct structures, indicating a well-mixed stellar population with a lack of significant recent merger activity. The galaxy's structure suggests a gravitationally relaxed system that is not currently undergoing major interactions or significant morphological disturbance.
