The galaxy appears as a centrally concentrated, relatively smooth object. There is minimal evidence of significant spiral arm structure or prominent dust lanes. The overall color profile suggests a relatively evolved stellar population, leaning towards redder hues, although some bluer regions are visible. The galaxy exhibits a generally elliptical morphology, appearing mostly round and showing no evidence of significant tidal disturbances or ongoing major mergers. There might be minor distortions, suggesting possible past interactions or minor mergers. The galaxy seems to be a high mass, high redshift quiescent galaxy.
