The galaxy appears to be a relatively smooth and centrally concentrated system. The light distribution is largely spheroidal in nature, with a distinct lack of spiral arm structure. The central region exhibits a bright, concentrated core, likely indicative of a significant stellar population. Proceeding outward from the core, the light gradually diminishes, forming a diffuse halo. The galaxy has a high degree of symmetry with only minor perturbations. The colors appear relatively uniform, indicating a stellar population of similar age across the system. Overall the galaxy is quite massive and forming stars at a low rate.
