The galaxy presents an overall elliptical morphology, appearing elongated with a smooth light distribution. The central region is considerably brighter, suggesting a concentrated nucleus. The galaxy's color gradient transitions from a yellowish-white core to a slightly bluer periphery, possibly indicating younger stellar populations in the outer regions. No prominent spiral arms or dust lanes are visible. The galaxy's structure appears relatively undisturbed, lacking evidence of significant tidal interactions or ongoing mergers, although some minor disturbances cannot be ruled out. The redshift indicates that this is a relatively distant galaxy, and its apparent size implies a substantial intrinsic physical scale. Integrated colors suggest a passively evolving galaxy, though low levels of star formation are likely still present.
