The galaxy presents as a centrally concentrated elliptical system. It exhibits a smooth, featureless morphology, with a bright, well-defined core that gradually fades into a more diffuse halo. The overall color appears slightly yellow. There is very weak evidence of a disk. The system does not appear to be undergoing any major merging activity, nor does it show any strong signs of tidal disturbances. The observed elongation suggests a shape somewhere between round and cigar shaped. The estimated stellar mass is quite high, likely around 4 x 10^10 to 5 x 10^10 solar masses. Considering its inferred mass, and overall elliptical morphology, star formation is expected to be at an overall low rate.
