The galaxy presents a generally smooth and centralized light distribution. It exhibits a dominant spheroid shape, with a concentration of older stars as evidenced by its yellow-reddish hue. There is little apparent disk structure or spiral arm presence. The galaxy displays a nearly circular morphology, with only slight deviations from perfect roundness. There is no obvious evidence of ongoing or recent major merger activity. A small amount of disturbance is possible within the galactic structure. The estimated size suggests a substantial but not exceedingly large physical extent.
