The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge, appearing bright and yellowish, suggesting a population of older stars. The galaxy's overall color profile indicates a relatively evolved stellar population, with a higher concentration of redder wavelengths. There is little evidence of significant dust lanes or spiral arm structures. The galaxy appears largely undisturbed, with no apparent signs of recent or ongoing major mergers. Subtle color variations are observed within the galaxy's halo, possibly indicating variations in stellar populations. Overall, this galaxy is consistent with an elliptical type galaxy with a moderate redshift.