The galaxy presents as a luminous, elliptical system, exhibiting a relatively smooth morphology. The central bulge is bright and appears spheroidal in shape, dominating the overall light profile. Proceeding outwards from the bulge, the light diminishes gradually, displaying a diffuse halo or envelope. There is some evidence of a flattened disk shape, although the bulge clearly dominates the galactic morphology. The light is slightly redder in the core than the outer region. There do not appear to be any signs of ongoing major merger activity or significant tidal distortions in the system's structure. There is the potential for a minor merger, due to slight disturbances in the disk region. No prominent dust lanes are visible, suggesting a relatively dust-poor environment. Overall, the galaxy presents as a relaxed, evolved system.
