The galaxy presents as a singular, relatively smooth structure. There is a concentration of luminosity toward the center, with a gradual decline in brightness toward the edges. The galaxy appears generally elliptical with the ratio of its major and minor axes being near unity. The color profile shows a relatively red hue, suggesting a population of older stars. There is no obvious evidence of spiral arm structures or prominent dust lanes. Based on the lack of significant morphological disturbance, the galaxy does not show any evidence of a recent major merger event. Minor asymmetry is present which may or may not be intrinsic to the object. The object appears generally consistent with an elliptical galaxy at a moderate redshift.
