The galaxy presents as an elliptical morphology, with a high degree of central concentration. It exhibits a smooth, relatively featureless appearance, suggesting a lack of significant spiral arm structures or prominent dust lanes. The color profile indicates a dominance of older stellar populations, with a yellowish-red hue. There is no obvious evidence of ongoing major mergers or tidal disturbances. A slight greenish tinge is visible, which could indicate some younger star formation, though it is not extensive. The overall shape appears roughly circular.
