The galaxy appears to be a relatively smooth, elliptical galaxy at a redshift of approximately 0.23. It exhibits a centrally concentrated bulge that fades into a less defined halo. There is little visible evidence of a prominent disk or spiral structure. The light distribution suggests a primarily older stellar population, possibly with ongoing but relatively low levels of star formation. There are hints of minor disturbances in the galaxy's overall morphology, but it does not appear to be undergoing a major merger or significant tidal interaction. It is more round than elongated. 
