The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge that dominates its overall structure. The light distribution suggests a high degree of sphericity, transitioning smoothly from a bright core to fainter, diffuse outer regions. The color profile indicates a population of older stars, evidenced by the yellowish to reddish hue of the galaxy's light. There is little evidence of spiral arms or significant dust lanes, supporting its classification as an elliptical galaxy. No apparent signs of recent or ongoing major mergers, although there are potentially very faint indications of minor tidal disturbances in the outermost regions, requiring further investigation. The galaxy's morphological structure suggests a dynamically relaxed system, typical of galaxies at a moderate redshift.