The galaxy appears to be a relatively smooth, elliptical system at a redshift of approximately 0.23, indicating a considerable distance. It exhibits a generally rounded morphology with no discernible spiral arms or a prominent disk structure. The galaxy's light profile suggests a fairly centrally concentrated luminosity, fading gradually towards the outer edges, with an effective radius of about 5.2 kiloparsecs. The color appears to be skewed towards the red end of the spectrum, indicating the presence of older stellar populations, and a relatively low rate of ongoing star formation. There is no evidence of any major mergers or significant tidal disturbances within the immediate vicinity of the galaxy. Its estimated mass is approximately 10^10.9 solar masses.
