The galaxy presents a somewhat elliptical morphology, appearing largely smooth and relatively undisturbed. Its light profile suggests a central bulge that fades gradually outward. There are no prominent spiral arms visible, nor are there any strong indications of significant tidal features or interactions. The color gradients across the galaxy hint at a centrally concentrated population of older stars, potentially indicating a more evolved system with comparatively subdued star formation. The overall color indices point toward a redder population suggesting older stellar populations and some dust obscuration within the system.