The galaxy appears to be a relatively smooth, single object with an elliptical morphology. It exhibits a concentrated light profile. There is no obvious presence of spiral arms or a prominent disk structure. There is some subtle evidence of a possible minor disturbance in the galaxy’s shape. The core is very bright, indicating a possibly dense stellar population or an active galactic nucleus. The galaxy exhibits a moderate redshift, suggesting it is a distant object. It emits most strongly in redder wavelengths of light. 
