The galaxy exhibits an overall elliptical morphology, with an aspect ratio suggesting it is viewed at an oblique angle rather than face-on. Its core is characterized by a smooth, concentrated luminosity profile indicative of an older stellar population. Surrounding this central region is a fainter, diffuse halo. There is slight disturbance in the disk. The galaxy has a redshift of approximately 0.13. Based on this information, this galaxy would have been actively forming stars about 1 billion years ago. The estimated mass of the galaxy is approximately 10^10 solar masses.