The galaxy appears to be a relatively smooth, centrally concentrated object. Its morphology suggests a dominant spheroidal component. There is very little evidence of distinct spiral arms or a well-defined disk structure, although a faint disk can not be ruled out. The light distribution is largely homogenous. The color is somewhat uniform across the galaxy, showing a slight redder hue to the center of the galaxy. This may be due to an older population of stars. There is no visual indication of major ongoing merger activity, though slight asymmetry or minor tidal features cannot be ruled out due to image resolution. The general roundness of the galaxy is a notable characteristic. Overall, the galaxy exhibits characteristics consistent with an early-type galaxy, most likely an elliptical or lenticular galaxy at moderate redshift.
