The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. It displays a yellowish-orange hue, suggesting an older stellar population. The galaxy appears mostly undisturbed with little to no disk-like features and with a very high degree of central symmetry. There may be a very faint indication of a minor interaction or tidal feature, as well as a close companion object nearby. The redshift data indicates that this galaxy is at a significant cosmological distance. The lack of distinct spiral arms or active star-forming regions, coupled with the color profile, suggests a relatively low specific star formation rate. Overall, this galaxy appears to be a massive, evolved system with a notable degree of central concentration.
