The galaxy appears to be an elliptical or lenticular type, displaying a smooth, centralized concentration of light. It exhibits a moderate redshift, indicating a substantial distance. The light distribution suggests a relatively old stellar population with minimal current star formation activity. The morphology is generally smooth, but with a possible minor tidal disturbance or interaction noticeable in a slight asymmetry. The galaxy's overall shape tends toward an intermediate roundness. There may be some evidence of a past minor merger event influencing its structure.
