The galaxy presents as a centrally concentrated, smooth object, exhibiting an elliptical morphology. The core is distinctly bright and yellowish-white in color, suggesting a population of older stars. Moving outward from the core, the color transitions towards a slightly bluer hue in the outer regions, possibly indicating a small presence of younger stellar populations. The overall structure displays a lack of spiral arms or significant disk features. There is a slight elongation visible, making it neither perfectly spherical nor highly flattened. No signs of ongoing major mergers or tidal disturbances are apparent upon initial inspection.
