The galaxy presents as an elliptical morphology, exhibiting a centrally concentrated, smooth light profile. The core region displays a yellowish-white hue, suggesting a population of older stars. Moving outward from the center, the color gradient transitions towards a bluish-white, indicating the presence of some younger stellar populations. The overall shape is generally elliptical with a slight deviation from perfect roundness. There may be a faint indication of a minor disturbance or asymmetry in the outer regions, but this is difficult to confirm definitively. No distinct spiral arm structures or significant dust lanes are visible. The galaxy appears relatively isolated, showing no obvious signs of a major merger event.
