The galaxy presents as an elliptical morphology, appearing largely smooth and featureless. The light profile indicates a centrally concentrated luminosity distribution. There is a hint of a slight extension in one direction, however, the overall shape is primarily round. The color is skewed toward the redder end of the spectrum, suggesting an older stellar population. No spiral arm structure or significant dust lanes are discernible. Based on the observed redshift, the galaxy's light has been significantly stretched, indicating a substantial distance. There is no evidence of any major ongoing merger activity, nor are any prominent tidal features apparent. The galaxy's color indicates that star formation may be somewhat suppressed.
