The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central region. The core exhibits a yellowish hue, suggesting an older stellar population. The galaxy appears to be moderately luminous, and is likely massive. The lack of distinct spiral arms or prominent dust lanes indicates it is not a spiral galaxy. There is little evidence of active star formation. The galaxy's morphology suggests it is not undergoing any major merging events, although minor disturbances can't be ruled out based on the image alone. The overall appearance points towards an evolved system.
