The galaxy presents as a somewhat diffuse, elliptical-like object with a bright, concentrated central bulge. The core exhibits a yellowish-orange hue, potentially indicating an older stellar population dominated by red giant stars. Moving outwards from the core, the light gradually diminishes, forming a more indistinct halo around the central region. Faint, blueish wisps or patches are subtly visible within the outer regions, hinting at regions of more recent star formation. The galaxy does not display any distinct spiral arm structure, but instead appears relatively smooth and unstructured. There's a suggestion of mild asymmetry or disturbance in the outer regions, potentially hinting at a past interaction or minor merger event.
