The galaxy presents an elliptical morphology. It exhibits a bright, concentrated central bulge that dominates its overall appearance. The light distribution appears fairly smooth, with no obvious spiral arm structures. The galaxy's color suggests a relatively old stellar population, with a notable absence of strong blue emission associated with active star formation. Faint, diffuse extensions are potentially visible, indicating the presence of a stellar halo or tidal features. The galaxy does not display prominent signs of an ongoing major merger, although some subtle irregularities might hint at minor interactions or disturbances in its past.
