The galaxy appears as a generally smooth, centrally concentrated object with a fairly elliptical morphology. Its light profile suggests a dominant bulge component, with little or no discernable disk structure. The galaxy exhibits a yellowish-orange hue, indicating an older stellar population with relatively little ongoing star formation. There are no significant signs of tidal disturbances or merging activity visible in the image. The lack of blue light suggests that the galaxy's star formation rate is suppressed. The overall appearance is consistent with that of an elliptical galaxy at a cosmological distance.
