This galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge that transitions into a diffuse halo. The galaxy has a generally round morphology, with very little apparent disk structure. There may be very minor disturbance within the structure. The color profile suggests an older stellar population, exhibiting yellowish hues. The galaxy is relatively isolated, with no apparent signs of ongoing major mergers or tidal interactions. Star formation is minimal. The galaxy is receding at a considerable fraction of the speed of light. The estimated size is relatively large for a galaxy at its redshift, indicating a significant physical scale. The luminosity is quite high. The stellar mass is estimated to be large.
