The galaxy presents as a relatively smooth, centrally concentrated object, likely an elliptical galaxy at a considerable distance. There is a distinct yellow-orange hue, suggesting an older stellar population. The object exhibits a round morphology, with only a slight elongation apparent. There appears to be a lack of significant spiral arm structures or dust lanes. No significant merging or tidal disturbances are visible in the image. There is some evidence of lower levels of star formation.
