The galaxy presents as a relatively smooth object, with a slight elongation. The light distribution appears centrally concentrated. There is no strong evidence of spiral arms or a prominent disk structure. The color is generally consistent across the galaxy, suggesting a relatively homogenous stellar population. There is a slight indication of a subtle disturbance in the galaxy's shape, although major merger events are not apparent. It appears to be an elliptical or lenticular galaxy at an approximate distance indicated by its moderate redshift. The object has a considerable mass and low star formation rate.
