The galaxy presents as a moderately luminous, elliptical morphology at a redshift of approximately 0.22, indicating a relatively large distance from the observer. It exhibits a smooth, centrally concentrated light profile, suggesting a dominant spheroid component. There is very little evidence of spiral arm structures or prominent dust lanes within the observable wavelengths. The galaxy appears relatively undisturbed, with no readily apparent signs of major recent merger activity or significant tidal features. The color indices show an overall redder hue, possibly indicative of an older stellar population with suppressed ongoing star formation. The galaxy exhibits a primarily round shape with no prominent elongations.
