The galaxy presents as an elliptical morphology, exhibiting a smooth, largely featureless profile. It possesses a bright, concentrated central bulge that gradually fades into an extended, diffuse halo. There is a slight elongation along one axis, suggesting a moderate degree of ellipticity, possibly of type E4-E5 on the Hubble sequence. The color appears relatively uniform across the galaxy, with a hint of bluer hues on the outskirts, possibly indicating some ongoing star formation. There's no prominent dust lane or spiral arm structure visible, corroborating the classification as an elliptical galaxy. Minor disturbances cannot be ruled out, although no major interactions are observed. The overall appearance suggests a mature system, having undergone significant dynamical relaxation.
