The galaxy presents a largely smooth, elliptical morphology. Its color profile is predominantly yellowish-orange, suggesting a stellar population that is dominated by older, redder stars. There is little evidence of significant dust lanes or spiral arm structures. The overall shape appears quite round, with no obvious elongation. No signs of ongoing or recent major merger activity are apparent, with a generally undisturbed structure. The light is centrally concentrated, with a gradual decrease in intensity outwards from the core, forming a halo. There is little evidence for ongoing star formation. The galaxy exhibits a notable luminosity at its observed redshift.