The galaxy presents as a centrally concentrated structure. The core region exhibits a bright, relatively smooth appearance, suggesting a high density of stars. The overall color profile appears somewhat muted, possibly indicative of an older stellar population. The galaxy's shape is generally elliptical but with a hint of a flattened profile. There may be a faint disk-like component, but it is poorly defined. There is no clear evidence of spiral arms or significant dust lanes. Faint, diffuse light extends outwards from the central region. The galaxy appears relatively undisturbed, with no obvious signs of a major ongoing merger, though subtle tidal features or minor disturbances cannot be ruled out.
