The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated light distribution. The core exhibits a yellowish hue, suggestive of an older stellar population. A subtle gradient toward a greenish-blue tint is observed in the outer regions of the galaxy, perhaps indicating the presence of younger stars or ionized gas. The overall shape is slightly elongated, with a moderate ellipticity. No distinct spiral arms or dust lanes are discernible. The galaxy appears relatively undisturbed, lacking prominent tidal features or signs of a major merger event.
