The galaxy presents a generally smooth and rounded morphology. Its luminosity profile appears centrally concentrated, with a gradual decrease in brightness extending outward. The core exhibits a yellowish-white hue, which may indicate an older stellar population. There are no obvious spiral arm structures or distinct dust lanes visible, suggesting a lack of significant ongoing star formation. The overall form is consistent with that of an elliptical galaxy. There are no signs of tidal disturbances or interactions with other galaxies in the immediate vicinity.
