The galaxy appears as an elliptical structure with a smooth, centrally concentrated light distribution. The core is bright and yellowish-white, possibly indicative of an older stellar population. Moving outward from the core, the light gradually diffuses, with some subtle color variations, suggesting a mixed stellar population. The overall shape is mostly round. There is a possible slight disturbance of a faint spiral arm. No strong tidal features or signs of a major ongoing merger are clearly visible.
