The galaxy presents a largely smooth morphology. Its shape is generally elliptical, appearing moderately elongated. The central region exhibits a concentrated, bright bulge which is yellow and orange. The color suggests an older stellar population in this region. This elliptical galaxy shows little evidence of active star formation and it has a stellar mass with log(M*/Msun) roughly around 11.25. Faint extensions of galactic material can be seen extending away from the central region. These extensions, combined with the observed elongation, suggest possible gravitational interactions, although the galaxy's overall structure remains largely undisturbed.
