The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. Its color is predominantly yellowish-orange, suggesting an older stellar population with fewer young, massive stars. The overall morphology indicates a system where the majority of stars are likely located in a spheroid, with little to no discernible disk component. There is no clear evidence of spiral arms or significant dust lanes, which are characteristic of disk galaxies. The light distribution appears fairly regular, with minimal signs of ongoing major mergers or tidal disturbances, although there is some evidence of a minor disturbance in the structure of the galaxy, which could imply that there has been a minor merger in the past. Based on its apparent magnitude and redshift, this galaxy is intrinsically very luminous. Based on its luminosity and color it is likely to be a massive elliptical galaxy.
