The galaxy exhibits a primarily elliptical morphology, with a relatively smooth and centralized light distribution. There is a bright, concentrated core, which suggests a potentially active galactic nucleus or a dense stellar population. Faint extensions or tidal features are visible that could be evidence of past minor interactions or mergers. The disk structure is difficult to resolve due to the strong bulge and the seeing conditions. Some disturbances in the outer regions hint at possible gravitational interactions with nearby galaxies.
